The galaxy presents an elliptical morphology, with a high degree of central concentration and a smooth light distribution. It is moderately elongated with the major axis extending in a northeast-southwest direction. The color index suggests a redder population of stars, indicative of an older stellar population and potentially lower star formation rate. Faint outer regions exist. There are no prominent dust lanes, spiral arms, or other features suggesting active star formation or recent mergers. The overall appearance points towards a relatively evolved system, consistent with an elliptical galaxy classification.
