The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a near-circular morphology, appearing generally rounded with a slight elongation. The central region is considerably brighter and bluer, suggestive of a concentrated population of younger, hotter stars or potential active galactic nucleus activity. The galaxy lacks any prominent spiral arm structures or obvious features indicative of ongoing major merger activity. A faint, diffuse halo of light extends outwards from the central region, gradually fading into the background. There is a hint of minor disturbance present, but overall the galaxy's structure seems stable and relatively undisturbed.
