The galaxy presents as a generally smooth, elliptical-like structure. The core exhibits a concentrated, bright, yellowish-white luminosity, suggesting an older stellar population dominating the central region. This central bulge is surrounded by a more diffuse halo of light that transitions to a bluish hue, hinting at the presence of younger stars or ongoing star formation, particularly in the outer regions. The overall shape appears moderately rounded, with a slight elongation. There is no apparent evidence of spiral arms or significant dust lanes; the galaxy exhibits a relatively uniform texture. There are no obvious signs of major merger activity or tidal disturbances, although minor asymmetries or subtle disturbances in the outer halo cannot be entirely ruled out with this image resolution.
