The galaxy appears as an elliptical or lenticular system, showing a smooth, diffuse light distribution. There is no prominent spiral arm structure or obvious dust lane obscuration. The light is more concentrated toward the center, creating a prominent bulge region. The galaxy exhibits a noticeable color gradient, with the central bulge appearing more reddish/yellowish and the outer regions showing a hint of bluer tones. This potentially indicates an older stellar population in the core and younger stars forming in the outer disk or halo. The overall shape seems slightly elongated, but not exceptionally so, trending toward a more spheroidal morphology. There is no clear evidence of ongoing major merging events or strong tidal disturbances, although subtle irregularities or minor features might be present upon closer inspection.
