The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears nearly circular. There is a bright, yellowish core that diminishes in intensity towards the outer regions. A subtle, diffuse halo surrounds the central core, exhibiting a slightly bluer hue than the central region. The faintness of the outer regions suggests a low rate of star formation. No signs of prominent spiral arms or distinct features such as bars or dust lanes are discernible within the galaxy's structure. There are no indications of ongoing major mergers or tidal disturbances affecting the galaxy's morphology.
