The galaxy presents as a spiral type, observed at an oblique angle, with a clear disk component. There is a substantial central bulge, exhibiting a yellowish hue, indicative of an older stellar population. Fainter spiral arm structures are visible emanating from the bulge, although the resolution limits a detailed tracing of their morphology. The arms appear relatively tightly wound. There are no clear indications of a strong bar feature. The galaxy demonstrates a notable degree of rotational symmetry. There does not appear to be any major ongoing merger activity.
