The galaxy presents as a spiral type, exhibiting well-defined spiral arm structures. Two main spiral arms are discernible, originating from a central bulge. The arms are relatively tightly wound. A bar feature bisects the central bulge. The bulge appears moderate in size, with an overall yellowish hue, suggesting a population of older stars. The spiral arms are bluer in color, indicative of ongoing star formation. There is no strong evidence of a recent major merger event.
