The galaxy presents as a relatively smooth object, likely an early-type galaxy or a spiral viewed face-on with a dominant bulge. It has a centrally concentrated luminosity profile, indicative of a dense stellar population at its core. The morphology appears mostly spheroidal, although there may be a hint of a disk component.

The color gradient transitions from a bluer hue in the outer regions to a redder hue in the central region. This could suggest an older stellar population dominating the core, with younger, bluer stars present in the outer regions, potentially associated with ongoing or recent star formation. The estimated size of the galaxy appears relatively moderate. There is some slight distortion in the shape, hinting at a possible past interaction.
