The galaxy exhibits a spiral morphology, with tightly wound spiral arms emanating from a central region. The spiral arms appear to be relatively well-defined, showing a distinct pattern. The central region appears to have a moderate bulge size. There's no indication of a strong bar structure bisecting the bulge. The color of the galaxy suggests a mix of stellar populations, with bluer regions within the spiral arms indicative of ongoing star formation. There is no significant presence of strong dust lanes obscuring the spiral structure. There is no evidence of any major mergers or significant tidal disturbances.
