The galaxy presents as a spiral type, oriented approximately face-on relative to our line of sight. Two distinct spiral arms are discernible, though they appear somewhat tightly wound. There's a clear central bulge, visually moderate in size relative to the disk. A bar structure is suggested within the central region, though potentially difficult to definitively characterize with the current image resolution. The spiral arms exhibit a clumpy appearance, indicative of active star formation regions. Overall, the galaxy appears relatively undisturbed, showing no obvious signs of major merging events, although subtle disturbances cannot be ruled out. The color profile suggests a mix of stellar populations, with a more yellow/red hue in the bulge suggesting older stars and bluer regions within the arms associated with younger, hotter stars. The overall morphology is consistent with an intermediate spiral type galaxy.
