The galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical or lenticular type given its overall morphology. There is a suggestion of interaction or a minor merger event ongoing, indicated by a slight asymmetry in the light distribution. One side appears slightly more extended and diffuse compared to the opposite side, with the presence of a bright, somewhat redder clump offset from the galaxy's main body. This feature could be either a satellite galaxy undergoing tidal disruption or a region of intense star formation triggered by the interaction. The bulk of the galaxy exhibits a yellowish-white hue, suggesting an older stellar population. The size of the galaxy appears modest. Overall, the galaxy does not appear to be a grand spiral or actively star-forming system, but rather a more evolved galaxy with subtle signs of recent or ongoing interaction.
