The galaxy appears as a somewhat elliptical, moderately sized object. The central region exhibits a concentrated, yellowish-orange hue, suggesting a population of older stars. Moving outward from the core, the color transitions to a more diffuse, greenish-blue. This coloration potentially indicates the presence of younger, hotter stars and ongoing star formation within the galaxy's spiral arms or outer disk.

The morphology shows evidence of possible tidal disturbances, with subtle asymmetries noticeable in the outer regions. Although no obvious merging companion is visible in this image, these asymmetries might suggest past or ongoing gravitational interactions with other galaxies. The overall structure doesn't appear to be a grand design spiral but more likely a flocculent or irregular spiral, or possibly a lenticular galaxy with faint arms.
