The galaxy presents as a single, relatively concentrated body. It appears primarily smooth in texture, with an elliptical morphology that is slightly more rounded than cigar-shaped, and not perfectly circular. There's no apparent spiral arm structure or bar feature. The core region presents as brighter, possibly indicating a high concentration of stars or an active galactic nucleus. There are no obvious signs of major disturbances indicating ongoing or recent major mergers with another galaxy. Faint, extended light may be present surrounding the galaxy. Based on the apparent color, the stellar population is likely dominated by older stars, emitting predominantly in the redder wavelengths, with an overall yellowish hue, suggesting a relatively low rate of ongoing star formation.
