The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears to be nearly circular. There is a suggestion of a slightly brighter central region, potentially indicating the presence of a galactic bulge or active galactic nucleus, though this is not definitively discernible from the image. The galaxy exhibits a color gradient, with a yellowish-white core fading to a slightly redder outer halo. There is no strong evidence of spiral arm structure, prominent dust lanes, or recent major merger activity. However, the overall morphology may exhibit a slight asymmetry. The galaxy's light distribution suggests a relatively evolved stellar population, consistent with a high fraction of the galaxy being smooth. The moderate size indicates the galaxy is likely massive. Star formation rate is low.
