The galaxy presents as a well-defined, moderately inclined disk galaxy. There is evidence of spiral arm structure emanating from the central region, which appears to be dominated by older stellar populations. The spiral arms display a bluer hue, indicating the presence of younger stars and ongoing star formation. A noticeable bulge component is present, and accounts for a substantial fraction of the light. There is no apparent disruption to the galaxy's morphology, suggesting it is not currently undergoing a major merger event, although there is the possibility of a small disturbance. The overall light distribution is relatively smooth within the disk, with no significant knots of star formation readily apparent, but it is clear that the galaxy is not quiescent. The galaxy appears to be relatively massive with an active star forming rate.