The galaxy presents as a luminous, centrally concentrated object with a generally smooth appearance. It exhibits a somewhat elliptical morphology, lacking any clearly defined spiral arm structures. The light distribution suggests a spheroidal component is dominant. There is a hint of a possible disk structure, but the bulge dominates the galaxy's overall light profile. Color gradients are subtle but present, with the core region appearing slightly more yellow than the outer regions. No obvious signs of ongoing major mergers or tidal disturbances are observed, although some minor irregularities may exist within its diffuse outer halo. The object does not display any prominent dust lanes or regions of intense star formation activity, and is plausibly classified as an early-type galaxy.
