The galaxy presents as a somewhat elliptical structure, exhibiting a relatively smooth and centrally concentrated morphology. The core region appears bright and yellowish, likely indicating a higher density of older stellar populations and possibly a supermassive black hole. Moving outward from the core, the galaxy displays a bluer hue, suggesting the presence of younger, hotter stars and ongoing star formation. Although there is no clear spiral arm structure, the outer regions of the galaxy display some faint, diffuse features that could be indicative of a disk-like component. There is no apparent strong tidal interaction or major disturbances observed, and any minor disturbances are difficult to discern given the resolution of the image. Overall, this galaxy appears to be a relatively quiescent system with ongoing, though potentially moderate, star formation.
