The galaxy appears as two distinct components: a larger, reddish entity, and a smaller, greenish-white companion. The primary galaxy exhibits a diffuse, relatively smooth morphology with a prominent red hue, suggesting a population dominated by older stars and/or significant dust obscuration. There may be evidence of tidal features or other disturbances in the form of asymmetries and irregularities in its outer regions, but overall it appears fairly round.

The smaller companion galaxy, positioned to the left, displays a more compact and bluer appearance. This suggests a younger stellar population and/or lower dust content. The blue-green coloration is prominent, indicating ongoing star formation.

The relative proximity and distorted morphology suggest that these galaxies may be interacting or in the process of merging. The overall impression is one of a dynamic system undergoing some form of gravitational interaction, leading to morphological disturbances and influencing the star formation rates within the galaxies. Further spectroscopic observations would be useful to ascertain the relative distances, radial velocities, and chemical compositions of these objects.
