The galaxy presents a morphology consistent with a spiral type, although the relatively low resolution of the image makes a definitive classification challenging. A distinct central bulge is visible, appearing moderately sized and relatively luminous. Surrounding the bulge, we observe a flattened disk structure. There is some indication of spiral arm structure, although it is not very clear or well defined. The disk exhibits a bluish tinge, suggestive of ongoing star formation within the galaxy. The galaxy does not appear to be strongly edge-on. The overall impression is of a spiral galaxy undergoing active star formation, with a substantial central bulge and some sign of spiral arms. There does not appear to be any major merger event occurring currently with this galaxy, however, the shape is somewhat disturbed, which may indicate that a minor merger event occurred in the distant past.
