The galaxy presents as a centrally concentrated object with a moderate degree of ellipticity. The primary body exhibits a relatively smooth texture, suggesting a lack of significant substructure or prominent spiral arms. The color gradient across the galaxy indicates a possible radial variation in stellar populations, with the central region appearing more yellow in tone and a slight gradient toward redder hues in the outer regions. There is a small object relatively close to the main galaxy body, but it is unclear at this resolution whether this object is gravitationally interacting with the main galaxy or not.
