The galaxy presents as a moderately bright object with a smooth, elliptical morphology. The light is fairly concentrated towards the center, with a gradual decrease in intensity towards the outer regions. It lacks any distinct spiral arm structures or prominent dust lanes. There appears to be a slight elongation, neither perfectly round nor extremely cigar-shaped. No signs of major mergers or significant tidal disturbances are apparent. Given its color and lack of distinct star-forming regions, the galaxy likely hosts an older stellar population with a relatively low ongoing star formation rate. 
