The galaxy presents an elliptical morphology with a smooth, diffuse light distribution. The core appears bright and concentrated, exhibiting a yellowish hue. There is a gradual decrease in luminosity from the central region outwards, lacking any distinct spiral arms or prominent features. The overall structure is predominantly spheroidal with a slightly elongated shape. The absence of dust lanes or distinct star-forming regions suggests a relatively quiescent galaxy, likely dominated by an older stellar population. Minor asymmetries and disturbances are subtle or absent. The galaxy appears to be an isolated system, showing no clear signs of ongoing or recent mergers.
