The galaxy presents an elliptical morphology, with a smooth, centrally concentrated light distribution. The core exhibits a bright, diffuse glow, suggestive of an older stellar population. The isophotes appear moderately flattened, indicating a moderate ellipticity. There is faint extension of stellar material beyond the main body of the galaxy, indicating a halo structure. The galaxy appears relatively isolated and shows no obvious signs of recent major mergers or tidal disturbances. There is no prominent dust lane or spiral arm structure visible. The color is redder towards the central bulge, transitioning towards bluer hues in the outer regions.
