The galaxy presents a relatively smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a well-defined disk structure. The light distribution suggests a centrally concentrated bulge. There is a possible very faint disk, with subtle color variations that hint at some minor star forming regions, though the galaxy appears predominantly composed of older stellar populations. There is no obvious evidence of a recent major merger or tidal disturbances; however, the galaxy is surrounded by several other galaxies that may be interacting, or dwarf galaxies. The galaxy's color suggests it has intermediate mass.