The galaxy presents as a relatively smooth, elongated structure. Its overall color appears to be a pale blue, indicating the presence of younger, hotter stars. The light distribution suggests a central bulge with an extended disk or halo. There's no clear evidence of spiral arms, but a slight asymmetry in the light distribution could suggest minor tidal disturbances or an ongoing merger event. The galaxy's shape is more cigar-like than circular, suggesting a classification as either an elliptical galaxy with some rotation or a lenticular galaxy viewed edge-on. There is a general concentration of light in the central regions, which fades toward the outer edges. The galaxy is relatively isolated.