The galaxy presents as a roughly elliptical structure. The core region displays a concentrated, bright, yellowish-white luminosity, suggesting a population of older stars. Moving outward from the core, the galaxy exhibits a gradient in color, shifting to a slightly greenish hue in the surrounding regions. There is little to no evidence of spiral arm structure. The outer edges are somewhat diffuse, exhibiting a smooth falloff in luminosity, implying a lack of significant recent star formation or dust obscuration. Overall, the galaxy appears to be relatively undisturbed, with no obvious signs of ongoing mergers or tidal interactions. The dominant morphological characteristic is that of an elliptical galaxy, potentially undergoing passive evolution.
