The galaxy exhibits a generally smooth morphology. Its shape is moderately circular, showing a slight deviation from a perfect circle but not appearing elongated. The central region is bright, suggesting a concentrated nucleus.

A subtle color gradient is observed; the central core appears more yellow, potentially indicating a population of older stars. The outer regions show a faint reddish hue, this may indicate the presence of cooler stars or dust absorption. There is little indication of spiral arm structures or prominent star-forming regions. Some minor asymmetry can be observed, but overall, the galaxy appears relatively undisturbed.
