The galaxy presents an elliptical morphology, appearing generally smooth and rounded in shape. It exhibits a concentrated central bulge that dominates its luminosity profile, with a gradual decrease in brightness towards its outer regions. The core is a bright, yellow-white hue which gradually fades towards the edges into a dimmer, redder shade. There is little evidence of spiral arm structure or significant dust lanes. The galaxy's overall color suggests an older stellar population, consistent with a reduced rate of ongoing star formation. Faint irregularities may be present in the outer halo, indicative of past minor mergers or tidal interactions.
