The galaxy presents a morphology suggestive of an elliptical or lenticular type. Its central region exhibits a high surface brightness, with a luminosity profile that appears to decrease gradually toward the outer edges. The isophotes are generally smooth. There is a slight deviation from perfect ellipticity, possibly indicating a minor interaction or internal structure, which is slightly more prominent in the bluer wavelengths. The color profile appears to be fairly uniform across the galaxy, trending toward a redder hue. This is consistent with an older stellar population. There is a faint suggestion of a tidal feature or a low-surface-brightness extension in one direction, indicative of potential past interaction. There also may be dust absorption in its center. 
