The galaxy presents as a generally smooth, elliptical morphology. It has a central, bright bulge that is roughly circular in appearance, with a yellow-white color suggesting an older stellar population. The outer regions of the galaxy appear less concentrated and somewhat fainter. There is some evidence of a slight disk-like structure, but no clear spiral arms are visible. The overall color gradient suggests a lack of significant ongoing star formation. The light is dominated by older stars, hence the relatively red color. There are no obvious signs of major tidal disturbances or ongoing mergers. The galaxy's roundness suggests it is closer to an E0/E1 classification on the Hubble sequence.
