The galaxy presents as a relatively smooth, centrally concentrated object. It appears to be elliptical in shape, with a moderate ellipticity. The color profile suggests an older stellar population, evidenced by the predominantly redder hues, indicating evolved stars. The galaxy does not exhibit any prominent spiral arm structure or significant dust lanes. There is no evidence of a recent major merger event, although subtle irregularities in its outer regions might suggest minor tidal interactions or accretion events in the past. Overall, the galaxy's morphology is consistent with that of a passively evolving system with a substantial stellar mass.
