The galaxy exhibits a morphology characterized by both smooth and featured components. There is a prominent central bulge exhibiting a smooth, concentrated luminosity profile, which transitions into a more diffuse, disk-like structure surrounding it. Evidence suggests the presence of internal features, possibly spiral arms or other structures, but these are faint. The bulge appears to be yellowish orange in color, with bluer hues in the surrounding disk, suggesting ongoing star formation. There is a slight asymmetry in the distribution of light, potentially indicative of minor tidal interactions or internal disturbances. Star formation appears to be low.