The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing more disc-like than perfectly spherical but also not particularly elongated, hinting at a potential intermediate shape. The light profile suggests a dominant bulge component, with a gradual fading of intensity towards the outer edges. 

There is some evidence of colour variation, the central region appearing more yellowish-red, suggesting an older stellar population and/or significant dust obscuration. The outer regions show a hint of bluer tones. No distinct spiral arm structures or prominent star-forming regions are visible. Any ongoing star formation is at a relatively low rate. There are no signs of any major disturbances or mergers; the galaxy appears generally undisturbed. 
