The galaxy presents as a centrally concentrated object, with a gradual decrease in luminosity outwards. The overall shape appears somewhat elliptical but is not perfectly spherical, showing a slight elongation. A faint disk-like structure may be present but difficult to discern. The galaxy exhibits a smooth texture, lacking prominent spiral arms or distinct star-forming regions in the available image resolution. The core is bright and unresolved, potentially indicating a dense stellar population or the presence of an active galactic nucleus, though further spectroscopic data would be required for confirmation. Color gradients are subtle, with a slightly bluer hue in the outer regions, suggesting the presence of younger stellar populations there compared to the redder, presumably older, stars in the central bulge. There is no obvious sign of ongoing major mergers or significant tidal disturbances.
