The galaxy presents as an elliptical morphology, appearing largely spheroidal with no discernable spiral arm structure. A smooth light distribution dominates, suggesting an evolved stellar population. The central region displays a higher concentration of light, appearing a slightly reddish-orange hue, possibly indicative of older, cooler stars and dust obscuration. The outer regions exhibit a subtle color gradient, transitioning to a slightly bluer hue, suggestive of some ongoing star formation. There is no evidence of significant tidal disturbances or major mergers, although minor asymmetries cannot be ruled out at this resolution. The object appears relatively isolated.
