The galaxy presents as a spiral type, though the arms are not sharply defined and appear somewhat flocculent. There is a noticeable central bulge, exhibiting a concentrated, yellowish hue, suggestive of an older stellar population. The spiral arms display a bluer tint, indicating the presence of younger, hotter stars, and ongoing star formation. Patches of faint dust lanes are tentatively observed within the arms, contributing to their irregular appearance. The overall morphology hints at possible gravitational interactions or recent minor merger events, evidenced by the disturbances within the spiral arm structure. Based on the color profile, the galaxy is actively forming stars at a moderate rate, with an estimated stellar mass is approximately 10^10 solar masses.
