The galaxy presents as a disk galaxy, viewed at an oblique angle, appearing somewhat elongated along its major axis. The central bulge exhibits a brighter, more concentrated light profile, with a subtly mottled texture indicating the presence of unresolved stellar populations or dust features. Emanating from the bulge is a fainter disk with a bluish tinge, possibly suggesting the presence of younger, hotter stars and ongoing star formation activity. The disk itself displays subtle variations in color and brightness across its extent. The morphological classification appears to lean towards a spiral type galaxy, despite not having tightly wound arms. There may be some kind of disturbance to the shape of this galaxy.
