The galaxy presents as a centrally concentrated object with a smooth morphology. It exhibits a roughly elliptical shape, appearing more "in between" round and cigar shaped, without a highly flattened disk structure. The galaxy displays a color gradient, transitioning from a yellowish-white core to a bluer, fainter outer region. No prominent spiral arms or bar structures are discernible. There are no obvious signs of a major ongoing merger, though subtle irregularities in the outer halo may indicate a past minor interaction or disturbance. The apparent absence of significant dust lanes or patches suggests relatively low levels of ongoing star formation, implying a galaxy dominated by an older stellar population.
