The galaxy presents a primarily smooth morphology with a slight ellipticity. The central bulge appears prominent and displays a concentrated, yellowish-white hue, potentially indicating an older stellar population. Fainter, bluer extensions are visible outwards from the central bulge, possibly hinting at the presence of a weak or poorly defined disk. These extensions suggest some ongoing star formation, although it appears to be at a low rate. There is no obvious evidence of spiral arm structure or significant dust lanes within the galaxy's visible extent. No major interactions or disturbances are apparent in the galaxy's structure. The galaxy appears generally isolated and relatively undisturbed.
