The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated luminosity profile, with the brightest region residing at the core. The shape approximates a round form. There is a suggestion of some minor disturbances, but without any major disruption to the overall structure. The galaxy presents a yellowish hue at its core, which transitions to a slightly bluer color towards the outer regions. The color gradient suggests potential differences in stellar populations, with older, redder stars likely dominating the core and younger, bluer stars in the outer regions. The size appears to be moderate, based on the imaging scale.
