The galaxy presents a smooth, elliptical morphology. There is no apparent disk or spiral arm structure visible in this image. The light is centrally concentrated with a fairly even intensity falloff toward the edges. It appears moderately rounded, not highly elongated or cigar-shaped. There is no obvious evidence of any recent or ongoing major merger activity, such as tidal tails or disrupted morphology, though some minor disturbances cannot be ruled out at this resolution. The galaxy appears relatively isolated within the observed field. The galaxy color seems to be redder, potentially indicating an older stellar population and a relatively low rate of star formation.
