The galaxy presents as a moderately luminous, spatially resolved object. It exhibits a generally smooth morphology with a slight elongation, suggesting it is not perfectly spherical but rather somewhere between round and cigar-shaped. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. Color gradients are subtle, with the core exhibiting a yellowish hue, and the outer regions appearing slightly redder. There is no readily apparent spiral structure or distinct disk component. Evidence of major mergers is not clearly visible; however, possible minor disturbances in the outer regions cannot be ruled out. Overall, the galaxy’s appearance is consistent with a relatively evolved system.
