The galaxy presents a largely smooth and rounded morphology. There is a dominant central bulge with a high degree of circular symmetry. The overall color profile suggests a relatively evolved stellar population, possibly containing a large fraction of older stars. There is a hint of asymmetry or minor tidal disturbance located to the southeast of the bulge, which may be indicative of past minor interactions or accretion events. The galaxy appears to be relatively isolated, with no other immediately apparent large galaxies nearby.
