The galaxy appears as a moderately bright, elliptical or lenticular type, with a smooth, diffuse light distribution, appearing mostly featureless. It exhibits a largely homogenous color profile across its structure, with the central region potentially being slightly brighter than the surrounding areas. There is no clearly visible spiral arm structure or distinct dust lanes. The galaxy's overall shape is nearly circular with some hints of a deviation toward an intermediate ellipticity. There may be some minor asymmetry suggesting a past interaction or disturbance, though its structure appears largely relaxed. It's luminosity appears to be moderately high, suggesting a galaxy of intermediate mass. The colors indicate a population of older stars and little to no ongoing star formation.
