The galaxy presents as a relatively smooth, centrally concentrated object with a slight ellipticity. Its core appears bright and luminous, indicative of a high stellar density. The overall color profile suggests a population of older stars, with a lack of significant blue light suggesting low levels of ongoing star formation. The galaxy does not display any prominent spiral arm structures, and instead appears to be of an elliptical morphology. There is no evidence of any major mergers or tidal disturbances in the vicinity. It presents with a high Sersic index, further supporting the classification as an elliptical.
