The galaxy presents a flattened, elliptical morphology. Its central region exhibits a bright, concentrated bulge that appears relatively smooth and featureless. Proceeding outward from the bulge, the galaxy displays a disk-like structure with a subtle color gradient, transitioning from a yellowish-white hue near the core to a slightly bluer tint in the outer regions. This suggests a distribution of stellar populations, with older, redder stars dominating the central bulge and younger, bluer stars populating the disk. There appears to be no strong evidence of a major ongoing merger event; instead, a smooth morphology and indistinct spiral arms imply that this is potentially an early type disk galaxy, or a late stage spiral galaxy where star formation has diminished. The lack of visible dust lanes further supports this assessment. The overall structure of the galaxy is elongated, but the roundness, it is neither perfectly circular nor highly elongated.
