The galaxy presents as a centrally concentrated spheroid with a smooth, relatively featureless appearance. The core region exhibits a bright, concentrated luminosity, suggesting a high density of stars in the central bulge. The overall color appears yellowish-orange, indicating a stellar population dominated by older, redder stars. There is a subtle decrease in luminosity and a slight color shift towards the periphery, hinting at a possible halo component. No distinct spiral arms or strong dust lanes are discernible, and the overall morphology points toward an elliptical classification or a lenticular galaxy viewed at a shallow inclination. The lack of significant morphological disturbances suggests it is likely a relaxed system, not undergoing any recent major mergers.
