The galaxy appears as a single, relatively smooth object with an elliptical morphology. It exhibits a concentrated, luminous core surrounded by a fainter, extended halo. The galaxy displays a redder hue in the central region, potentially indicating an older stellar population or significant dust obscuration. No distinct spiral arms or prominent star-forming regions are discernible. The overall color profile suggests the presence of both evolved stars and possible ongoing, albeit subdued, star formation. There is no strong evidence of any major mergers or tidal disturbances in its immediate vicinity. Based on its smooth appearance, it is likely an early-type galaxy, possibly an elliptical or lenticular galaxy.