The galaxy presents as a centrally concentrated, elliptical-like structure. It appears largely smooth in texture, with a notable lack of distinct spiral arms or prominent dust lanes. The core region exhibits a bright, condensed luminosity, suggesting a significant concentration of stars within the galactic nucleus. A gradual decrease in surface brightness is observed moving outward from the center towards the galactic periphery. The overall color profile leans towards yellow-red, indicative of an older stellar population dominated by evolved stars, with only a hint of bluer light. There is no compelling visual evidence of ongoing major merger activity or significant tidal disturbances. The morphological appearance strongly suggests classification as an elliptical or lenticular galaxy.
