The galaxy presents as a largely featureless, smooth object. It is elliptical in shape, exhibiting a high degree of roundness. The central region is a bright, concentrated yellow core. There is a gradual decrease in luminosity moving outwards from the core, with no distinct spiral arm structures or prominent dust lanes visible. The galaxy appears isolated, with no signs of ongoing major mergers or significant tidal disturbances, though there is some evidence of minor asymmetry in the outer regions. The color suggests an older stellar population, implying relatively low current star formation. The overall structure suggests a mature galaxy with a large stellar mass.
