The galaxy presents as a single, centrally concentrated object with a smooth, featureless appearance. Its overall shape appears roughly round. There is a bright central region suggesting the possible presence of an active galactic nucleus or a high concentration of stars in the core. The color gradient suggests that the central region is dominated by older stellar populations, while the outer regions may contain slightly younger, bluer stars. No distinct spiral arms or bar structures are visible. There is no evidence of any major mergers or significant tidal disturbances affecting its structure. The faintness of the outer edges of the galaxy suggest a relatively quiescent stellar formation rate. 
