The galaxy presents as a relatively smooth, elliptical-like system, exhibiting a centrally concentrated light profile. The core region is bright and appears yellowish-white, potentially indicating an older stellar population. Moving outwards from the core, the galaxy gradually fades, displaying a less intense, diffuse halo. There's a slight flattening observed, with a suggestion of a disk-like structure. The color transitions from the yellowish-white core to a more neutral, possibly slightly bluish-white hue in the outer regions. No distinct spiral arms or dust lanes are immediately apparent within the galaxy's structure. The overall morphology suggests a galaxy undergoing, or that has already undergone, significant evolutionary processes, resulting in a more quiescent state.
