The galaxy presents as a somewhat flattened spheroid with an elliptical profile. Its central region exhibits a bright, concentrated core indicative of a possible nucleus or bulge. Diffuse, extended structures are visible beyond this core, implying a disk component that is viewed at a relatively high inclination. There is some indication of faint, tidal-like features extending from the main body, suggesting possible past interactions or mergers. Colors vary across the galaxy, with the central region appearing more yellow and the outer regions with hints of blue, which might reflect varying stellar populations and/or dust content. A slight asymmetry is observed in the surrounding regions of the galaxy, suggesting minor disturbances.
