The galaxy presents an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The core region appears bright and yellowish, possibly indicating an older stellar population. The isophotes are generally elliptical, although there's a slight deviation from perfect ellipticity. The overall color gradient suggests a radial change in stellar population, with the outer regions appearing slightly bluer. There is evidence of some disturbances or asymmetric features within the galaxy's structure, potentially hinting at past or ongoing interactions. No distinct spiral arm structures or significant dust lanes are visible. The galaxy seems relatively isolated, with no obvious nearby companions or tidal features strongly suggestive of a recent major merger.
