The galaxy presents a predominantly smooth, elliptical morphology. It exhibits a concentrated central bulge, which graduates into a less defined, more diffuse halo. There appears to be some internal structure and subtle colour variations within the galaxy; however, these features are not highly pronounced. The galaxy has a fairly symmetrical profile, with a hint of elongation. Some minor, irregular features may indicate minor gravitational interaction. The colours are consistent with an evolved stellar population with lower specific star formation. Overall, the galaxy appears to be a fairly massive system.
