The galaxy presents as a relatively smooth, elliptical structure. It exhibits a central concentration of light that gradually diminishes towards the outer edges, suggesting a well-established stellar population. There is a slight elongation in its overall shape, deviating minimally from a perfectly circular form. No distinct spiral arms or prominent dust lanes are visible, which supports the elliptical classification. There appears to be minimal sign of recent or ongoing merging activity. The galaxy's color profile is predominantly yellow and red, indicating the presence of older stars and a low rate of current star formation.
