The galaxy appears to be a relatively compact elliptical or lenticular system. Its morphology is dominated by a smooth, centrally concentrated bulge. The light profile suggests a gradual decrease in surface brightness from the core outward. Some subtle asymmetries and faint extended light may be present, suggesting minor tidal interactions or past mergers. The galaxy exhibits a yellowish hue, indicative of an older stellar population, with relatively little active star formation occurring within the visible extent of the galaxy. A small amount of bluer light is visible near the core, possibly indicating some star formation. There does not appear to be any presence of defined spiral arms.
