The galaxy presents as a relatively smooth, elliptical morphology. Its color profile suggests a predominantly older stellar population, with a yellowish-white hue dominant throughout the galactic body. There is little to no evidence of spiral arm structures or significant dust lanes. The galaxy's overall form is elongated, appearing more 'in-between' round and cigar-shaped. Faint, diffuse light extends from the central region, gradually fading into the background sky. There is no clear sign of recent or ongoing major merger activity. Slight asymmetry might suggest minor gravitational interactions or internal disturbances but is indistinct. The overall light distribution is relatively even.
