The galaxy exhibits a morphology consistent with a spiral structure, although the arms appear somewhat tightly wound. The central bulge is prominent and exhibits a yellowish hue, suggesting an older stellar population. The spiral arms show a bluer color, indicating the presence of younger, hotter stars and ongoing star formation. There is a clear disk-like structure. The galaxy shows signs of some irregularities and possible disturbances, as the shape is somewhat asymmetric. There may be an indication of minor tidal interactions or a past merger event. The overall appearance suggests a galaxy undergoing relatively modest star formation activity. The galaxy is of intermediate size and luminosity for its type.
