The galaxy presents as a relatively smooth, elliptical structure. The main body of the galaxy exhibits a bright central bulge, displaying a yellow-orange hue. This suggests an older stellar population dominating the core. Fainter, bluish regions are visible surrounding the bulge, potentially indicating areas of more recent, albeit subdued, star formation within the galactic disk. A distinct redder region is apparent on one side of the galaxy, possibly a region of dust obscuration or a concentration of older, redder stars. The overall shape is somewhat rounded but appears to show a slight elongation, hinting at a disk component. There may be faint signs of tidal disturbances, such as a faint plume or asymmetry in the outer regions, which could be indicative of past or ongoing interactions with another galaxy. A significant portion of the galaxy seems smooth, though there is some disturbance in the outer regions.
