The galaxy presents as a centrally concentrated, elliptical-like structure. The core exhibits a bright, relatively uniform luminosity profile, suggesting a high density of stars. The overall shape is predominantly round, with no apparent spiral arms or significant disk-like features. The outer regions of the galaxy gradually fade into the background, indicating a smooth density gradient. There is no visible evidence of major mergers or significant tidal disturbances. A slight color gradient exists, with the central region appearing more yellow than the outer regions, possibly indicating a difference in stellar population or dust content. Star formation appears to be low due to the distinct lack of blue light. The smoothness of the light distribution suggests that this is an evolved galaxy with a substantial spheroidal component.
