The galaxy presents a generally smooth morphology, with the majority of its light concentrated in a central bulge. The overall shape is elliptical, appearing more elongated than perfectly circular. A faint, diffuse disk surrounds the central bulge. There are no prominent spiral arms, bars, or dust lanes visible. The color appears to be largely homogeneous across the galaxy, indicating a primarily older stellar population, with redder colors more prominent. There is no apparent active galactic nucleus or significant star formation activity. There is some minor visible disturbance.
