The galaxy appears as a relatively smooth, elliptical object. It exhibits a high degree of radial symmetry, with a gradual decrease in luminosity from the center outwards. There is no visible spiral structure, bar, or prominent dust lanes. The galaxy's color profile suggests a population of older stars, exhibiting colors indicative of minimal on-going star formation. There are some faint disturbances that suggest a small chance of minor merging with a small galaxy, however, this galaxy appears to be a relatively relaxed system. The overall morphology is consistent with that of an early-type galaxy.
