The galaxy presents a generally smooth, elliptical morphology, appearing relatively undisturbed. Its shape is more rounded than elongated, with only a slight suggestion of a cigar-like form. The color profile shows a central concentration of yellowish-white light, suggesting a population of older stars. This central region is surrounded by a more diffuse halo of bluish-green light, hinting at the presence of some younger stellar populations or possibly ongoing star formation, albeit at a low rate. There is marginal evidence of a minor disturbance in its structure, but it appears relatively quiescent, showing no clear signs of a recent major merger or significant tidal interactions. The galaxy's overall structure is quite regular and centrally concentrated.
