The galaxy presents as a relatively smooth object with a distinctly elliptical morphology. It exhibits a noticeable central bulge that appears to be the brightest region. The overall color profile suggests a population of older stars. The disk, if present, is not clearly resolved; the galaxy exhibits a somewhat cigar-shaped appearance, with no apparent spiral arms. No indications of major tidal disturbances or ongoing mergers are observable in this image, although there may be some minor asymmetry. The galaxy has a moderate angular size. Based on the color profile and lack of spiral arms, the star formation rate is estimated to be low.
