The galaxy presents as a largely amorphous, centrally concentrated luminous object. It exhibits a smooth overall morphology with no apparent spiral arm structures or distinct features immediately visible. The core region is significantly brighter than the outer regions, suggesting a high concentration of stars toward the galactic center. The light gradually decreases towards the periphery, with an elliptical shape. The color appears to be primarily yellowish-white, indicating a population dominated by older stars with minimal active star formation. There is no obvious evidence of significant dust lanes or recent major merger events disrupting the morphology. The overall impression is of a relatively evolved galaxy, potentially of an elliptical or lenticular type.
