This galaxy presents as a spiral type, displaying a relatively well-defined disk structure. The spiral arms appear somewhat tightly wound, and are discernible, emanating from a central bulge. The central bulge is moderately prominent, displaying a bright, concentrated light profile. The disk exhibits a bluer color, suggestive of ongoing star formation activity. There are several prominent HII regions along the spiral arms, indicating regions of intense star birth. There is evidence of a possible bar structure within the central regions of the galaxy. There are some subtle irregularities in the disk that suggest possible minor interactions or internal disturbances.