The galaxy presents as a moderately luminous object with a generally smooth morphology. The central region exhibits a concentrated, bright core, potentially indicative of an active galactic nucleus or a dense stellar population. The light distribution transitions gradually from this bright core into a more diffuse halo, with some subtle extensions or features that suggest possible tidal interactions or minor disturbances in the galaxy's structure.

The overall color profile suggests a mixed stellar population. The central core is more yellow, implying older stars. Surrounding regions show a bluish tint, which could signify younger stars or star formation regions. The estimated size suggests a substantial galaxy. The galaxy does not show any strong signs of a major ongoing merger or dramatic tidal disruption.
