The galaxy presents as a relatively smooth, rounded structure. A bright central bulge is evident, indicating a concentration of older stars in the galaxy's core. The outer regions display a slightly more diffuse and blueish hue, hinting at the presence of younger stellar populations and ongoing star formation, although perhaps not at a very intense rate. No prominent spiral arms or bar structures are clearly discernible. There appears to be no major ongoing merger activity or significant tidal disturbances. Overall, the galaxy seems to be an evolved system with moderate star formation.
