The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central region. The core exhibits a bluish-white hue, suggesting a population of hotter, younger stars and potentially active star formation. Moving outward from the core, the light becomes less concentrated, transitioning into a more diffuse halo. This outer region appears slightly more reddish than the core, indicating a potentially older stellar population. There is a slight elongation of the galaxy's shape; it is more in-between rounded than it is cigar shaped. There is no clear evidence of a spiral arm structure, and the overall morphology suggests a relatively undisturbed system, though faint tidal features or minor disturbances cannot be ruled out with this image. The apparent size of the galaxy is small, indicating it is at a considerable distance. There does not appear to be any major merger activity occuring.
