This galaxy exhibits a smooth morphology with a moderate ellipticity. The light distribution appears concentrated towards the center, suggesting the presence of an aging stellar population, particularly in the redder wavelengths. There is a lack of defined spiral arms or prominent dust lanes. A subtle color gradient is observed, with the core region appearing more yellow-red and the outer regions showing a slightly bluer tint. This suggests a possible difference in stellar population age and composition between the center and the outer parts. Evidence of any recent major mergers or strong tidal interactions is not seen.
