The galaxy presents a moderately elliptical morphology, exhibiting a smooth and relatively featureless appearance across its central region. A concentrated bulge dominates the luminosity profile, with a gradual decrease in brightness towards the outer edges of the disk. Subtle color gradients are observed, with the central bulge appearing slightly more yellow/red-shifted, potentially indicating an older stellar population compared to the bluer hues in the outer disk. There is no discernable presence of distinct spiral arms or a prominent bar structure. The general shape appears to be disturbed with some areas being slightly more dense.