The galaxy exhibits a clear spiral structure, with prominent arms emanating from a central bulge. The arms appear somewhat tightly wound. Two dominant arms are visually apparent, though finer detail regarding tertiary structures are difficult to resolve. The bulge appears relatively moderate in size in proportion to the disk. There is no obvious bar structure visible within the central region. The overall color gradient suggests a mix of stellar populations, with bluer tones in the spiral arms indicative of ongoing star formation and redder hues in the central bulge potentially associated with older stellar populations. The galaxy does not appear to be strongly interacting or undergoing a major merger, with a relatively undisturbed disk and arm structure. Evidence of minor disturbances cannot be ruled out. The estimated size suggests this is a relatively large spiral galaxy.
