The galaxy presents as an elliptical structure. It exhibits a relatively smooth morphology, with no prominent spiral arms or bar features readily apparent. The light distribution is concentrated towards the center, indicating a significant bulge component. There is no sign of any active galactic nuclei in the image. There is not enough visible distortion to suggest a recent major merger event; however, some minor disturbances cannot be ruled out. The galaxy appears to be generally rounded in shape, as opposed to elongated or cigar-shaped. The apparent size is small, and there are no signs of tidal tails or streams. Based on the color profile, star formation is likely low within the galaxy.
