The galaxy presents as a centrally concentrated object, generally elliptical in morphology with a noticeable radial gradient in luminosity. The core is bright and unresolved at this resolution, indicative of a high stellar density or potentially an active galactic nucleus. Moving outward from the core, the luminosity decreases. There is faint, diffuse material surrounding the central region, extending approximately two to three times the radius of the bright core. The galaxy does not appear to have any distinct spiral arms or a well-defined disk structure. There may be some indication of tidal disturbances or minor asymmetries in the outer regions, but these are not pronounced. The colour distribution suggests relatively uniform stellar populations throughout the galaxy, with perhaps a slight reddening towards the core. Overall, the galaxy appears relatively isolated and undisturbed.
