The galaxy presents as a somewhat diffuse, yellowish object. It does not display a well-defined spiral or elliptical structure, but exhibits a more irregular morphology. A significant fraction of the light seems concentrated in a more intense and seemingly separate region within the galaxy's broader structure. The overall color indicates a stellar population that has evolved over a considerable timeframe, with fewer young, blue stars. There are hints of disturbance, particularly with the uneven distribution of light, possibly indicating that it is undergoing interaction or a merging process. The galaxy appears to be relatively massive, given its brightness and potential size. The very low star formation rate is consistent with an older stellar population.
