The galaxy presents as a single, centrally condensed object. The overall morphology appears relatively smooth, lacking prominent spiral arms or a distinct bar structure. The light distribution suggests a spheroidal shape, with a high degree of circularity. There is a clear concentration of luminosity towards the galactic center. The color gradient indicates a possible radial variation in stellar populations, with the core exhibiting a more yellowish hue compared to the slightly bluer outer regions, suggesting a higher proportion of older stars in the center. There is no evidence of a recent major merger or tidal disturbances in its immediate vicinity, as the structure appears largely undisturbed and symmetrical. Faint, diffuse extensions or a very subtle disk component may be present, but further investigation would be required to confirm this. The galaxy appears to be relatively isolated.