This galaxy exhibits a spiral morphology, presenting a disk-like structure. There appears to be a central bulge, although it is not overly prominent in comparison to the disk. The spiral arms are well-defined, with two dominant arms that extend outwards from the central region, showing a medium to loose winding pattern. The galaxy displays some degree of internal structure and hints of ongoing star formation, as indicated by the slightly irregular appearance of the spiral arms. Evidence of a bar structure is also observed, bisecting the central bulge. There may be a minor interaction or disturbance evident in the distortion of the disk. Overall, the galaxy presents as a fairly typical spiral galaxy, viewed at a slight angle.