The galaxy presents as a fairly smooth, elliptical object. Its core is a bright, concentrated yellowish-white, indicating a significant population of older stars. The outer regions of the galaxy exhibit a bluer hue and a somewhat elongated shape. There is a faint hint of a disk-like structure or spiral arms, but they are not well-defined. The galaxy is moderately massive and has a relatively low star formation rate. There is no obvious evidence of a major merger or tidal disruption. The galaxy is in the intermediate stages of a spheroidal transformation.
