The galaxy presents as an elliptical form, exhibiting a centrally concentrated luminosity profile, indicative of a spheroidal component. The light distribution becomes increasingly diffuse toward the outer regions. Its color index appears redder, suggesting a stellar population dominated by older stars. The galaxy appears to be experiencing a possible minor disturbance or a merger event, as evidenced by the slight irregularities on one side, and what seems to be a smaller companion object. Given its morphological characteristics, it can be classified as an elliptical galaxy with signs of interaction. It also appears to be fairly massive with low star formation rates.
