The galaxy presents as an elliptical morphology with a smooth, centralized bulge dominating its structure. The light profile indicates a high degree of concentration towards the center.  The color gradient suggests the core region exhibits a yellowish hue, potentially indicating an older stellar population. Moving outwards, the galaxy displays a slight reddening, which may point to some dust obscuration or a shift in stellar population towards cooler, redder stars. There is no readily apparent spiral arm structure or star forming regions are visible in this image. The lack of defined features indicate a relatively quiescent state of star formation within this system. The overall shape appears slightly elongated, though not dramatically so. No signs of tidal disturbances or interactions are apparent.
