The galaxy presents as a single, somewhat symmetrical object. It is dominated by a concentrated central region, appearing a warm yellow hue suggesting a population of older stars. The galaxy exhibits a smooth overall appearance, with no obvious spiral arm structures or distinct features. The shape appears roughly circular in projection, suggesting a classification as an elliptical galaxy or a face-on disk galaxy with a prominent bulge. The galaxy exhibits a color gradient with the core appearing more yellow, which is consistent with a greater concentration of older stars in the central region. There is no evidence of significant ongoing star formation within the galaxy. No signs of tidal disturbances or mergers can be visually identified.
