The galaxy appears to be a relatively smooth, elliptical system. It presents a notable central bulge with a redder hue, possibly indicative of an older stellar population and dust obscuration. The outer regions exhibit a gradual decline in surface brightness. There is an extended, somewhat flattened disk-like component surrounding the bulge, showing a slight blue tint suggesting the presence of younger stars or ongoing star formation at a reduced rate. The overall shape appears more in between round and elliptical rather than distinctly one or the other. There are no obvious signs of major disturbances, merging activity or tidal tails present in the immediate vicinity. The galaxy has a concentrated core, contributing to the overall smooth appearance.
