The galaxy appears as a moderately bright, roughly elliptical object. The core region displays a concentrated luminosity with a yellowish-orange hue, which gently diffuses outward. There is a subtle indication of a disk-like structure surrounding the core, showing a faint greenish tint at its edges. The outer regions show a smooth and gradual decrease in brightness, lacking any prominent spiral arms or significant dust lanes that are readily discernible. Overall, the galaxy exhibits a relatively homogenous texture and does not appear to be undergoing any major merger events or tidal disturbances. Its shape leans towards a roundness, though some slight elongation is noted. The colour profile suggests a relatively evolved stellar population with limited ongoing star formation, though some degree of star formation is weakly implied by the greenish tint.
