The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal. The light distribution peaks centrally, with a gradual falloff towards the periphery. There's a subtle elongation, suggesting it is not perfectly spherical. The color profile displays a redder hue in the central region, potentially indicating an older stellar population concentrated in the galactic nucleus. The outer regions exhibit a slightly bluer tint, possibly from younger stars, but is very weak. No distinct spiral arms or prominent dust lanes are observed. The overall structure appears relatively undisturbed, with no signs of major mergers or significant tidal interactions. There might be minor disturbances, but there is no obvious sign of a merger. The galaxy appears to be a quiescent system, without bright star formation regions.
