The galaxy presents as a centrally concentrated object with a generally smooth appearance. There is some suggestion of a very faint, diffuse disk-like structure surrounding the brighter central region, though its features are not well defined. The galaxy's color profile appears relatively homogenous, with a slight shift towards redder hues in the central core. There is no obvious spiral arm structure or significant dust lane features visible. The overall morphology suggests a relatively evolved system, with the light profile being consistent with an elliptical or lenticular galaxy. While the majority of its light is concentrated in the center, the distribution of light is generally round. There is no evidence of an ongoing major merger, although very faint, minor disturbance cannot be completely ruled out.
