The galaxy presents a roughly elliptical morphology, with a noticeable bulge component. The central region exhibits a yellowish hue, which suggests an older stellar population. The outer regions display a bluer tint, possibly indicating the presence of younger, hotter stars and ongoing star formation. These outer regions also appear less smooth and more granular, potentially showing spiral arm structures, although these are not well-defined. The overall structure appears somewhat disturbed, perhaps due to past interactions or mergers. The galaxy has an estimated size of approximately 6 kiloparsecs across its half-light radius.
