The galaxy presents as a relatively smooth, lens-shaped structure. There is a distinct central bulge that appears to be comprised of older stars. The galaxy shows an intermediate axial ratio, appearing somewhat elongated but not significantly flattened. Faint spiral arm structures may be present but are not well defined. The color gradient across the galaxy suggests a concentration of older, redder stars in the central bulge, while the outer regions show slightly bluer hues, potentially indicating the presence of younger stellar populations. Some degree of minor disturbance is possibly observable. Overall, the galaxy seems to be a moderately massive system with a low star formation rate, potentially evolving towards a quiescent state.
