The galaxy presents as a primarily smooth, elliptical-like structure. The light distribution appears centrally concentrated with a bright, yellowish core that gradually diffuses outwards. There is little evidence of spiral arm structures or distinct features within the galaxy. The overall morphology suggests an evolved system, potentially an elliptical galaxy with a significant population of older stars. A subtle extension or tidal feature might be present on one side, suggesting a possible interaction or past merger event, although this is not very prominent. The color profile indicates a generally older stellar population.
