The galaxy appears as a centrally concentrated, moderately luminous object with a generally smooth morphology. A bright, yellowish core suggests a concentration of older stars, possibly a bulge. Extending outward from the core is a fainter, bluish disk-like structure. There appears to be very little, if any, pronounced spiral arm structure; rather, the overall form is more lenticular. The galaxy presents a moderate degree of ellipticity, appearing somewhat flattened. Subtle irregularities in the outer regions suggest possible minor gravitational interactions or past merger events, though the overall structure is relatively undisturbed. The blue coloration in the outer regions indicates ongoing, albeit not intense, star formation activity.
