The galaxy appears as a luminous, centrally concentrated object, likely an elliptical or lenticular galaxy given its smooth, featureless morphology. A pronounced bulge dominates the galaxy's structure, exhibiting a yellowish-white hue, suggesting a population of older, evolved stars. The isophotes of the galaxy are generally round, with a slight deviation towards an intermediate shape. There is no apparent disk structure or spiral arm features. The galaxy exhibits a faint, extended halo surrounding the central bulge, which fades into the background sky. There are some minor indications of disturbances, but overall the structure appears relatively relaxed and unperturbed. The galaxy's color indices imply that it has moderate star forming properties.
