The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth and centralized light distribution. Its shape is elongated, approaching an intermediate state between round and cigar-shaped, with a slight deviation from perfect circularity.

Color gradients within the galaxy suggest potential variations in stellar populations. The central region displays a concentration of yellow-red hues which fade out into a pale blue hue on either side. This may indicate an older, more evolved stellar population centrally, with a ring of younger, hotter stars present in the galaxy.

There are also visible disturbances in the form of a slight asymmetry, suggestive of a recent or ongoing interaction with a smaller object. This disturbance manifests as a subtle warp or tidal feature extending towards the southern part of the galaxy.
