The galaxy presents as a primarily smooth, elliptical object. The light distribution appears relatively uniform, with a concentration of luminosity towards the galactic center. There is no apparent spiral arm structure or significant dust lane obscuration visible. The overall shape is somewhat rounded, though not perfectly circular, presenting an intermediate ellipticity.

There is evidence of a possible minor disturbance within the galaxy's structure, potentially indicative of a past or ongoing minor interaction or accretion event. This is subtle, not presenting a distinctly warped morphology.

The galaxy exhibits a color gradient, appearing bluer at the core and becoming redder toward the outer regions. This could suggest varying stellar populations or dust content across the galaxy. The overall color suggests a population of older stars.
