The galaxy presents as a relatively smooth object, exhibiting a slightly elliptical morphology. Its overall structure appears largely featureless, lacking prominent spiral arms or a distinct bar. The central region displays a bright, concentrated bulge, which gradually fades into a more diffuse halo. Color gradients are subtle, with a bluish hue near the center potentially indicating a younger stellar population or ongoing star formation in this region. The outer regions appear redder, suggesting a population of older, cooler stars. There is no visually apparent evidence of significant tidal interactions or ongoing mergers, and the general form of the galaxy is indicative of a stable, relatively undisturbed system. The galaxy's profile suggests a disk component is likely present but not particularly dominant.
