The galaxy presents an elliptical morphology, appearing largely smooth with a notable concentration of light towards its center, suggesting a prominent bulge. The overall shape is elongated, displaying a moderate cigar shape. There are no apparent signs of major mergers or significant tidal disturbances affecting its structure. Color gradients indicate a bluer periphery compared to the yellowish central region. This suggests the presence of younger stellar populations in the outer parts of the galaxy, with potentially older, redder stars dominating the core. There is some evidence of minor internal features or slight irregularities within the extended disk. The estimated size is on the order of several kpc. The galaxy is relatively luminous.
