The galaxy appears as a relatively smooth, centrally concentrated object, elliptical in shape and likely devoid of prominent spiral arm structures. It exhibits a slight elongation, suggesting a possible transition between a spheroidal and a more lenticular morphology. The galaxy displays a radial color gradient, with the central region appearing more yellow/orange than the outer regions, indicating a potentially older stellar population concentrated in the core. There is no visible dust lane and no other clear morphological irregularities, although there might be some subtle disturbances. Based on its luminosity and apparent lack of active star formation, this galaxy is likely a massive, relatively quiescent system. There may be signs of minor interaction with nearby objects. The galaxy's overall smooth appearance supports the classification as an early-type system.
