The galaxy presents a slightly elongated, elliptical morphology. A smooth, diffuse light distribution dominates, suggesting a relatively old stellar population. There is a subtle hint of bluer light concentrated towards the central region, possibly indicating a small amount of ongoing star formation there. Faint, disturbed structures are visible. A possible minor disturbance in the symmetry of the light, that suggest tidal interactions or a minor merger event in its past. The galaxy appears to be of relatively low mass with a small effective radius. It exhibits a faint red color overall, consistent with a low star-formation rate and a dominant population of older stars.
