The galaxy appears to be elliptical in morphology, exhibiting a smooth, centrally concentrated light profile. The core region is significantly brighter and exhibits a yellowish hue, indicating a population of older stars. Moving outward from the core, the color transitions to a slightly bluer shade, suggesting the potential presence of a younger stellar population in the outer regions. The galaxy demonstrates a largely featureless appearance, with no clear evidence of spiral arms or significant dust lanes. The overall shape appears close to circular, with a minor deviation towards an elongated form. There are no obvious signs of ongoing mergers or major tidal disturbances affecting its structure, suggesting that this is a relatively relaxed system. A slight asymmetry could indicate minor interactions with other galaxies, but this is not conclusive from the image.
