The galaxy presents as a relatively smooth, elliptical morphology. The light distribution appears centrally concentrated, exhibiting a gradual decline in surface brightness from the core outwards. There is a noticeable color gradient, with the core appearing more yellow/orange, suggestive of an older stellar population. The outer regions appear bluer, hinting at the presence of younger stars, though this component is not prominent. No distinct spiral arms or bar structures are discernible. The overall shape is generally round, with no significant signs of tidal disturbances or major mergers. The galaxy exhibits a low star-formation rate.
