The galaxy presents as an elongated structure, appearing cigar-shaped. Its central region is dominated by a bright, yellowish core, suggesting a concentration of older stars. The luminosity profile appears relatively smooth, with a gradual decrease in intensity from the core outwards. Fainter, diffuse extensions are visible at both ends of the galaxy's major axis. These extended features indicate the presence of a stellar halo or tidal debris. There seems to be some minor disturbance within the galaxy. Overall, it appears to be a fairly massive galaxy with moderate star formation.
