The galaxy presents as a somewhat smooth, elliptical-like structure, appearing largely spheroidal in shape. A bright, centrally concentrated bulge dominates the galaxy's morphology. Fainter, diffuse light extends outwards from the core region. There is a subtle color gradient, with the central region exhibiting a slightly redder hue than the bluer outer halo. No distinct spiral arm structures or dust lanes are clearly visible, suggesting the possible absence of a well-defined disk or ongoing major star formation within the primary body of the galaxy. There might be some minor disturbances and signs of a potential past merger event; however, the overall appearance is not exceptionally disturbed, with a high probability of its current structure being unperturbed. The object exhibits significant luminosity. The estimated size of the galaxy is a few kiloparsecs in radius.
