The galaxy presents as a moderately luminous, elliptical structure. The central region exhibits a concentrated, bright core, suggestive of a high stellar density. The overall color appears to be slightly redder, potentially indicating an older stellar population and a relatively quiescent star formation rate. There is a smooth, gradual decrease in luminosity from the core outwards, with no obvious spiral arm structures or dust lanes visible. The object shows a somewhat round morphology. There's no evidence of significant tidal disturbances or ongoing major mergers. 
