The galaxy presents as an elliptical morphology, appearing mostly smooth with a concentrated central bulge. The light distribution suggests a high degree of symmetry. A slight elongation is observable, deviating marginally from a perfect circle. The core exhibits a yellowish hue, indicating an older stellar population. The outer regions show a subtle shift toward reddish tones, which may represent older stars, dust, or the effects of redshift. No spiral arm structure or significant dust lanes are discernible. There is no evidence of any major tidal disturbances or ongoing mergers with another galaxy. The galaxy shows characteristics of an evolved system with little to no active star formation apparent in the image.
