The galaxy presents as a relatively compact, centrally concentrated object. Its overall morphology appears smooth and largely featureless, lacking prominent spiral arms or a distinct disk structure. The light distribution suggests a spheroidal shape, approaching circular symmetry, with a gradual decrease in surface brightness from the core outwards. There are no obvious signs of tidal tails or other distortions indicative of recent major merger activity, though subtle irregularities or minor disturbances are not entirely ruled out at this resolution. The core region appears relatively bright.
