The galaxy presents a spiral morphology, viewed at an oblique angle relative to its disk. The spiral arms are not sharply defined but appear flocculent and somewhat patchy in color, suggestive of ongoing, but not particularly intense, star formation regions distributed throughout the disk. The central bulge region is moderately prominent, with a smooth, concentrated appearance and a yellowish-white hue, indicating a population of older stars. There may be evidence of a bar-like structure crossing the bulge. The disk shows some signs of possible disruption or interaction, although not overtly dramatic, indicated by the slight asymmetry in the arm structure. Dust lanes are subtle, but faintly visible along the inner edges of some spiral arm segments.
