The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits a bright, concentrated luminosity, suggesting a high density of stars in the galactic nucleus. Moving outwards from the core, the light gradually diminishes, forming an extended halo. The galaxy appears to be slightly elongated, deviating from a perfect circle, with an intermediate shape leaning towards a more rounded rather than cigar-shaped morphology. There is a subtle hint of a disk-like structure, yet it is not pronounced and appears subdued. Overall, the galaxy's structure appears relatively undisturbed, with little to no evidence of significant tidal interactions or ongoing mergers. In terms of color, the central region appears yellowish.
