The galaxy presents as a somewhat smooth, disk-like structure, but with noticeable internal features suggestive of spiral arms. Its overall shape is elongated, trending toward a cigar-like appearance rather than a perfectly circular disk when viewed at this orientation. The galaxy's color profile indicates a relatively older stellar population, exhibiting a reddish-yellow hue concentrated towards the center of the galaxy, which could be due to a higher density of older stars. There may be some slight evidence of a minor gravitational disturbance, but the overall structure appears relatively undisturbed. The galaxy's light profile suggests ongoing, but subdued, star formation activity.
