The galaxy presents as a somewhat amorphous, extended object with a dominant, centrally concentrated luminosity. The central region exhibits a yellowish-orange hue, potentially indicative of an older stellar population. There appears to be a secondary concentration of light offset from the main body, suggestive of a possible tidal feature or a smaller companion galaxy undergoing interaction. The overall morphology appears disturbed, showing some signs of asymmetry. Given the color profile, it is likely that star formation activity is low, although some bluer regions imply pockets of more recent stellar birth. The galaxy shows a smooth light distribution with some suggestion of a diffuse disk-like structure. There is a significant merging aspect that appears to be due to tidal disturbances, suggesting the possibility of minor mergers. The estimated size is relatively small, but it exhibits a complex structure, including a rounded feature and a more elongated component.
