The galaxy presents a predominantly smooth morphology, with an apparent lack of significant spiral arm structure or prominent dust lanes. The object exhibits a somewhat elliptical shape, though it deviates from a perfect circularity, appearing slightly elongated. Its color profile suggests a population of older stars, leaning towards the redder end of the spectrum. Overall, the galaxy appears relatively undisturbed, showing no major signs of on-going merging activity or tidal distortions.
