The galaxy presents as a relatively smooth, centrally concentrated object. The light distribution suggests a morphology consistent with an elliptical galaxy, lacking any discernible spiral arm structure or prominent dust lanes. Its shape is generally round. There is very little evidence of recent or ongoing mergers or significant tidal disturbances. The object appears to have a well-defined core with a gradual decrease in luminosity towards its outer regions, indicating a single galactic body and not two interacting objects, despite the irregularity in its distribution of light. The colour suggests an older stellar population with a relatively low star formation rate. The low rate of star formation is consistent with what would be expected from a galaxy of this type and morphology.
