The galaxy presents as a spiral type, viewed at a significant angle from face-on. The central bulge appears moderately prominent and exhibits a yellowish hue, suggestive of an older stellar population. Spiral arms are well-defined, displaying a predominantly blue color, indicative of ongoing star formation. The arms appear to be fairly tightly wound, with a notable presence of two dominant arms. Indications of a bar structure are present, although not exceptionally strong. The overall morphology suggests the galaxy is a relatively undisturbed spiral, without major signs of ongoing or recent major mergers, although there might be some minor tidal features visible.
