The galaxy presents as a spiral type, with moderately tightly wound spiral arms that are clearly observable. Its disk exhibits a high degree of inclination relative to our line of sight, appearing somewhat elongated. A prominent central bulge is visible. The galaxy exhibits color variations, with bluer regions concentrated within the spiral arms, likely indicating active star formation, and a more yellow/red hue towards the central bulge, suggestive of an older stellar population. There are some minor visible irregularities or disturbances, suggesting possible interactions with other objects. There is a hint of a bar-like structure within the inner regions. Overall the galaxy is slightly disturbed but has a relatively well defined spiral structure.
