The galaxy presents a generally smooth, elliptical morphology. It appears to be moderately luminous, with a concentrated central bulge exhibiting a bright, near-white glow. The galaxy’s overall shape appears largely undisturbed, displaying no obvious signs of recent major mergers or strong tidal interactions, however, minor disturbances cannot be ruled out.

There are some subtle color variations in the outer regions of the galaxy, suggesting the presence of distinct stellar populations. A faint hint of bluer emissions can be seen on one side of the bulge, potentially indicative of ongoing, albeit subdued, star formation activity in that area. The size of the galaxy seems relatively compact.
