The galaxy presents as a single, centrally concentrated object. Its morphology appears largely spheroidal, exhibiting a smooth, featureless profile with a high degree of roundness. There is no indication of spiral arms or a prominent disk structure. A slight elongation is observed in the object's shape, although it maintains a mostly circular appearance. The galaxy exhibits a color gradient, with a yellowish hue concentrated towards the central region, transitioning to a redder halo at its outer edges. There is no discernible evidence of significant ongoing star formation, which is consistent with a well-evolved stellar population. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or major mergers. However, there is some slight irregularity in the outer isophotes that may indicate minor disturbances.
