The galaxy presents as a centrally concentrated object, exhibiting a largely smooth morphology. The color profile suggests an older stellar population dominating the central bulge, which appears yellow-orange. Fainter blue light can be observed in the outer regions, implying more recent star formation is occurring on the outskirts. There is no clear spiral structure or prominent disk component visible. The overall shape appears more elliptical, with no indication of major disturbances or mergers. However, there is a possible very minor disturbance located in the outer regions. It is likely that this galaxy has a relatively high mass, considering its luminosity and lack of significant ongoing star formation in the nuclear region.
