The galaxy presents a concentrated, centrally-brightened morphology. It has a smooth appearance. The central region appears to be yellowish in color, suggesting an older stellar population. There is a very slight asymmetry, although it is generally elliptical. Subtle color variations throughout the galaxy indicate variations in stellar populations or dust content. There is no evidence of a significant disk structure, spiral arms, or ongoing major mergers. It appears to be an intermediate-sized galaxy. The absence of prominent blue regions suggests a relatively low star formation rate. Overall, it is a relatively undisturbed galaxy, but the asymmetry suggests there might be a small companion or recent past minor merger.
