The galaxy presents as an elliptical-type system, exhibiting a smooth, centrally concentrated luminosity profile. The core region displays a yellowish-white hue, potentially indicative of an older stellar population and lower star formation rates. Surrounding the core is a more extended halo of bluish-white light, suggesting the presence of some younger, hotter stars, though this population appears less dominant than the older stars in the core. The galaxy shows a somewhat elongated shape, with a relatively flattened structure. Some level of disturbance can be seen in the disk, but there is no strong evidence of tidal tails or other strong merging features. The overall appearance is relatively undisturbed, suggesting that this galaxy has undergone minimal recent major interactions.
