The galaxy appears to be a relatively smooth, elliptical or lenticular type. It exhibits a concentrated central bulge that is bright and yellowish in color, suggesting an older stellar population. The galaxy's light profile decreases steadily outwards from the center, with no visible spiral arms or prominent dust lanes. The outer regions of the galaxy have a faint, diffuse halo, possibly composed of older stars and globular clusters. The overall shape appears nearly circular, indicating minimal rotational support. There is no evidence of major ongoing mergers or significant tidal disturbances. The colors suggest a population dominated by older stars, with relatively low levels of recent star formation.
