The galaxy appears as a relatively smooth, elliptical structure. It exhibits a central bulge that is bright and concentrated, with a gradual decrease in luminosity towards the outer regions. The overall shape is somewhat elongated, but not highly flattened, indicating a likely classification as an elliptical galaxy of intermediate ellipticity, possibly an E4 or E5 on the Hubble sequence. Faint hints of a disk-like structure are apparent. There is a subtle color gradient visible, with the core appearing slightly yellower/whiter than the outer regions, suggesting an older stellar population in the center. There are hints of some very minor disturbances in its morphology, and may have had minor interactions with another galaxy in its past, but otherwise it appears to be stable. There are faint spiral arms present but the image is very faint. The galaxy possesses a significant mass and exhibits moderate star formation.
