The galaxy presents an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. There is a prominent bulge, indicated by the yellow hue, which likely signifies an older stellar population. The outer regions of the galaxy appear less concentrated and slightly bluer, hinting at the presence of some younger stars or ongoing star formation, albeit at a relatively low rate. The overall shape is closer to round than cigar-shaped but not perfectly circular. No signs of major tidal disturbances or ongoing mergers are apparent. The galaxy appears relatively isolated and undisturbed.
