The galaxy presents as a generally smooth object, elliptical in shape, with a slight elongation. It appears to lack any significant spiral arm structure or prominent dust lanes. The core exhibits a bright, concentrated luminosity, suggesting a high stellar density and potentially an active galactic nucleus.

The color gradient shifts from a yellowish-white center, indicative of an older stellar population, to a slightly bluer halo. The bluer tint in the outer regions may suggest ongoing, but relatively low level, star formation activity. There is no obvious visual disturbance to the main body of the galaxy. Based on the observed features, it may be classified as an elliptical galaxy undergoing modest star formation.
