The galaxy exhibits a primarily smooth morphology, with a likely central bulge. It demonstrates an overall elliptical appearance, trending slightly towards a more rounded shape. There is evidence of an ongoing or recent interaction or merger event, indicated by a noticeable asymmetry and some disturbance in the surrounding galactic halo. The core region displays a reddish hue, possibly indicating an older stellar population. A bluer region is visible towards the bottom of the galaxy, suggestive of younger stars or active star formation regions. Overall, the galaxy's light profile suggests a evolved system undergoing interaction.
