The galaxy presents as a relatively smooth, concentrated object with an elliptical morphology. There is some indication of a slight elongation, but it is generally rounded in appearance. The galaxy appears to be dominated by an older stellar population, with a yellowish-red hue indicative of lower star formation activity and a lack of significant dust obscuration. There might be some minor disturbances in the galaxy's structure, possibly indicating a past or ongoing minor interaction, but there is no evidence of a major merger or significant tidal features.
