The galaxy presents a morphology that suggests an intermediate stage between a pure elliptical and a spiral galaxy. It displays a prominent central bulge region that appears relatively smooth and concentrated, exhibiting a yellowish hue suggestive of an older stellar population. Extending outwards from the bulge, there is a fainter, more diffuse disk component. The disk shows subtle hints of structure, potentially indicating the presence of spiral arms or dust lanes, but these features are not sharply defined. There is some irregular structure and disturbance, which could be tidal arms. There may be a small amount of star formation present. The galaxy is relatively isolated, with no obvious signs of major interactions or mergers with other galaxies.
