The galaxy presents with a morphology suggesting a system undergoing interaction or a recent merger event. A larger, more prominent structure exhibits a yellowish-white hue, indicative of an older stellar population. This central body appears somewhat amorphous with a slightly elongated form, lacking the well-defined spiral arm structure typically seen in undisturbed disk galaxies.

Adjacent to this primary body, a smaller, bluer component is visible. The blue color suggests a younger stellar population possibly triggered by the interaction. This distinct clump implies ongoing or recent star formation. The overall system displays a moderate luminosity and has an estimated size in the kiloparsec range.

Faint distortions or tidal features might be present, though image resolution limits definitive identification. There's a slight asymmetry in the distribution of light around the central region, potentially supporting the interaction scenario. Based on the color indices, the galaxy is likely to have a moderate mass and a comparatively low rate of star formation relative to its mass.
