The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high degree of concentration with a bright core. There is a faint but discernible outer halo extending beyond the core, gradually fading into the background sky. The overall color appears to be dominated by light from older stellar populations, with a slightly reddish hue, although some bluer colors can be seen in the central areas. There is no apparent evidence of strong spiral arms, a bar structure, or significant dust lanes. The galaxy does not appear to be undergoing any major merging events or significant tidal disturbances based on its morphology.
