The galaxy presents as a centrally concentrated system with a relatively smooth, diffuse morphology. The core exhibits a distinctly reddish hue, which could indicate an older stellar population or significant dust obscuration in the central region. The galaxy appears mostly round, with no apparent spiral arm structures or bar features visible in this image. A faint, extended halo surrounds the central region, exhibiting a bluer color gradient compared to the core. The overall smooth appearance suggests it is likely an elliptical galaxy, potentially in a relatively quiescent state with a low star formation rate. No signs of major merger events or significant tidal disturbances are obvious, although subtle asymmetries or minor disturbances within the halo cannot be ruled out without higher resolution imaging.
