The galaxy appears as a relatively smooth, elliptical structure. There is little evidence of spiral arms or significant disk-like features. The central region exhibits a higher surface brightness concentration, characteristic of a galactic bulge. The outer regions gradually fade into the background, suggesting a decreasing stellar density with increasing radius. The galaxy exhibits a slight ellipticity, appearing somewhat elongated rather than perfectly spherical. Faint indications of minor disturbances or interactions are suspected; however, no major mergers or significant tidal features are discernible. The color gradient is subtle, with a possibly redder hue in the central region compared to the periphery, which could indicate an older stellar population at the core. The overall morphology indicates a mature galaxy, likely with suppressed star formation.
