The galaxy presents a generally smooth appearance, with a concentration of light toward the center suggesting a bulge. The overall shape is approximately round, though subtle variations in luminosity hint at underlying structure. Fainter, diffuse features extend outwards from the central region, possibly indicating a disk component or tidal disturbances. The color profile displays a gradient from yellowish hues in the core to bluer shades in the outer regions, suggestive of a transition from older stellar populations in the center to younger, star-forming regions in the periphery. There are some very faint and minor disturbances in the lower parts of the galaxy. These disturbances could be caused by a minor merging event.
