The galaxy presents as a relatively smooth, elliptical-like structure. The core exhibits a concentrated, bright yellowish-orange color, suggesting a significant population of older stars. The outer regions of the galaxy appear more diffuse, with a subtle gradient towards a greener hue, possibly indicating the presence of a younger stellar population or ongoing star formation at a lower rate. There is little evidence of spiral arm structure or significant dust lanes. The galaxy appears largely undisturbed, without prominent signs of tidal interactions or a recent major merger. Its overall shape appears nearly round, lacking a pronounced elongated structure.
