The galaxy presents an elliptical morphology, appearing predominantly smooth with a centrally concentrated light profile. The light is primarily yellow and white. The shape exhibits an intermediate roundness, neither perfectly spherical nor highly elongated. There is evidence of a potential minor disturbance in the galactic structure, possibly indicating a past or ongoing interaction. A merger may be occuring within the galaxy structure. The overall color suggests an older stellar population with a relatively low rate of ongoing star formation. The galaxy appears to be a single object without any major companions or significant tidal features.
