The galaxy presents as a face-on spiral with a noticeable bulge. Spiral arms are readily apparent, exhibiting a relatively tight winding pattern. The color profile is indicative of ongoing star formation, with a bluer hue in the spiral arms and a yellower, more evolved population in the central bulge. There is no obvious evidence of a strong bar structure, but a subtle asymmetry in the spiral arm distribution hints at a possible weak bar or interaction. The galaxy appears relatively undisturbed, with no major signs of tidal tails or morphological disruption associated with a recent major merger.
