The galaxy presents as a largely featureless, smooth elliptical type object. The central region exhibits a concentrated luminosity with a golden hue, suggesting a population of older stars. A slight ellipticity is observed, but it appears generally rounded. There is no apparent spiral structure or prominent dust lanes. Color gradients suggest a redder core, potentially indicating a higher concentration of older stars toward the center. Overall, it is a relatively compact and quiescent system. A smaller, fainter object is visible in close proximity, potentially indicating a satellite galaxy or background object. No signs of significant tidal interactions or recent mergers are evident in the primary galaxy.