The galaxy presents as a single, fairly uniform entity with a centrally concentrated brightness profile. It exhibits a generally elliptical morphology with a slight deviation from perfect roundness, appearing more disc-like than spherical, but without a clear, defined spiral structure. The galaxy's color is predominantly yellow-white, suggesting a significant population of older stars. There is a lack of distinct blue regions, implying a relatively low rate of ongoing star formation throughout the galaxy. Faint disturbances in shape might be hints of minor gravitational interaction. There is no clear evidence of strong tidal tails or other indicators of a major merger event in progress.
