The galaxy presents as a single, centrally concentrated object with a generally smooth morphology. The light profile appears roughly circular, trending towards elliptical, with no obvious spiral arm structures or a prominent disk. The core region exhibits a bright, yellowish hue, suggesting an older stellar population or significant dust obscuration. A faint, diffuse halo of greenish light surrounds the central region, potentially indicative of a younger stellar population or ongoing star formation at a low rate. No signs of tidal tails, mergers, or significant disturbances are apparent.
