The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a concentrated luminosity gradient, appearing as a bright, reddish core. Moving outward from the core, the light gradually diffuses into a less intense halo. There is a slight hint of bluer hues towards the outer edges. No distinct spiral arm features or prominent dust lanes are discernible. There appears to be no ongoing major merging activity or significant tidal disturbances, though there is a subtle irregular shape on its left side. The galaxy's overall morphology suggests it is likely a relatively evolved system, with a moderate amount of star formation taking place within.
