The galaxy exhibits a predominantly smooth morphology, with a high degree of roundness. There is no apparent bar structure or spiral arm structure. The central region appears as a concentrated bulge, displaying a yellowish-white hue indicative of an older stellar population. Fainter, diffuse blue light extends from the center, hinting at regions of ongoing star formation. There are no obvious signs of tidal disturbances or mergers, suggesting the galaxy is relatively isolated and undisturbed. The overall color gradient shifts from yellow-white in the core to slightly bluer hues in the outer regions.
