The galaxy presents as a relatively smooth, elliptical-like structure. There is a bright, concentrated central bulge, with the light appearing to gradually diminish outwards, showing a diffuse halo. The galaxy exhibits an elongated shape, appearing more cigar-shaped than perfectly round. There are no obvious spiral arms or prominent dust lanes visible. There is a suggestion of slight disturbance on one side, but overall the galaxy appears relatively undisturbed with no signs of a major merger. The color profile suggests a population of older stars. Star formation is relatively low.