The galaxy appears as a centrally concentrated object, with light distribution suggestive of an elliptical morphology. It is somewhat elongated in shape, but largely appears rounded. There appears to be a smooth falloff of light intensity from the center outwards, lacking any clear spiral arm structure or prominent features. There is no evidence of major tidal disturbances or ongoing mergers, although some minor asymmetry in its outer regions cannot be ruled out. The object exhibits a notable blue hue, implying the presence of relatively young, hot stars. The galaxy has a somewhat diffuse appearance, lacking sharp boundaries.
