The galaxy presents an overall disk-like structure, viewed at a significant inclination. There is evidence of spiral arm features although they appear somewhat patchy and not particularly well-defined. A central bulge is present, with a moderate size relative to the disk. The galaxy's color profile suggests the presence of both older stellar populations in the bulge, indicated by a yellowish hue, and some ongoing star formation in the disk, noted by the slightly bluer color in the spiral arm regions. The dust lanes within the disk are subtle but visible. There are no signs of major mergers or strong tidal disturbances, though minor irregularities may suggest some past interactions. The overall form of the galaxy is moderately asymmetrical.
