The galaxy presents as a lenticular or possibly an elliptical system, viewed nearly edge-on from our perspective. It exhibits a smooth, diffuse luminosity profile with a slight color gradient, appearing more reddish towards the core and subtly bluer towards the outer edges of the disk. This color variation could be indicative of ongoing, albeit limited, star formation activity in the outer regions. The overall morphology is elongated and cigar-shaped, with no prominent spiral arm structures or distinct features suggestive of a major ongoing merger event. There are no observable dust lanes or other significant disruptions to its symmetry. The galaxy appears relatively isolated, with no obvious signs of tidal interactions with nearby companions in this image.
