The galaxy appears to be a relatively smooth, centrally concentrated system. Its morphology is largely spheroidal, with little discernible disk structure. The light distribution suggests an elliptical galaxy, possibly an E2 or E3 type based on its observed ellipticity.

The galaxy exhibits a color gradient, appearing more yellow/orange towards the core, suggesting an older stellar population dominated by evolved stars. Fainter, bluer regions may be present in the outer reaches, hinting at some recent star formation activity, although this is not a dominant feature. There is no visual evidence of ongoing major mergers or significant tidal disturbances, but a subtle irregularity in its overall shape could indicate a minor interaction in its past. The galaxy's overall luminosity suggests it is a massive system.
