The galaxy presents a spiral morphology, exhibiting well-defined, tightly wound spiral arms. A prominent central bulge is observed, with an apparent moderate size relative to the disk. The galaxy displays a notable disk component, viewed at an angle that is not quite face-on, but not fully edge-on either. The presence of a bar structure is suspected but not clearly visible. Star formation is evident, as indicated by the blue color in the spiral arms. There may be signs of minor disturbances or interactions, but these are not prominent. The nucleus of the galaxy has a distinct color. Overall, the galaxy appears to be a relatively massive system.
