The galaxy presents as a centrally concentrated object, exhibiting a smooth, largely featureless morphology. Its overall shape appears close to circular. The light distribution is dominated by a bright, relatively compact core, which fades gradually outwards into a more diffuse halo. There is no discernible spiral structure or distinct disk component visible in this image. Subtle color gradients are observed, with the central region appearing somewhat bluer than the outer regions, potentially indicating a higher concentration of younger, hotter stars in the nucleus, compared to older stellar populations in the halo. There is no apparent tidal distortion or interaction with nearby galaxies, based on the morphology observed. The object appears relatively isolated. The galaxy lacks pronounced dust lanes or other signs of significant dust obscuration.
