The galaxy exhibits a generally elliptical morphology, appearing somewhat flattened along one axis, suggesting a possible disk-like structure. The central region displays a high concentration of luminosity, indicative of a bright galactic nucleus or bulge. Moving outward from the core, the light intensity decreases gradually.

There is a subtle presence of faint, diffuse features extending from the main body of the galaxy, possibly indicative of tidal tails or other forms of galactic interactions or disturbances. I see a slight asymmetry in the outer regions, again suggesting a possible past merger event. The colour of the light ranges from blue to red across the object.&#x20;
