The galaxy presents as a relatively smooth, elliptical-like structure. There is a noticeable concentration of light towards the center, suggesting a prominent bulge. The galaxy exhibits a gradual decrease in luminosity from its core towards the outer regions, with no distinct spiral arm features visible. There are some blue colored clumps that can be seen towards the outskirts, suggesting regions of star formation. The galaxy appears to have a fairly regular shape, with no evidence of major tidal disturbances or ongoing mergers.
