The galaxy presents as an elliptical or lenticular type. Its central region displays a bright, concentrated bulge, exhibiting a smooth texture with no apparent dust lanes. Fainter and more diffuse light extends outward from the core along a relatively even plane. The morphology is more elongated than circular, but it does not appear to be a thin, edge-on disk. There is faint evidence of possible tidal distortion, though it is minor. This may be due to a past interaction. The color profile indicates a population of older stars, particularly in the central bulge, as indicated by the yellow and red light. Star formation is likely minimal, with only faint evidence of blue light in the surrounding areas.
