The galaxy presents as a fairly smooth and centralized object. Its overall shape appears elliptical, tending slightly towards an in-between rounded form, lacking a highly defined disk structure. It exhibits a dominant central bulge characterized by a yellowish-white hue, suggesting an older stellar population within the core. The galaxy lacks apparent spiral arms or other distinct features associated with ongoing star formation. There is no evidence of significant tidal distortions or ongoing merger activity. The overall color profile leans towards the redder end of the spectrum, which is consistent with a galaxy with a more evolved stellar population and a lower star formation rate.
