The galaxy presents as a relatively compact structure with a prominent central bulge that appears yellowish-white in color, suggesting an older stellar population. Fainter and more diffuse spiral arms extend outwards from the bulge, exhibiting a reddish hue, possibly indicative of dust lanes or regions of ongoing star formation. The overall morphology seems to be that of a spiral galaxy, although the spiral structure is somewhat indistinct. The galaxy is not perfectly circular, showing a slight ellipticity with a tilted orientation relative to the observer. There is no obvious signs of strong tidal disturbances or ongoing major mergers, although subtle asymmetries in the outer regions can be seen.
