The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, somewhat compact structure. Proceeding outwards from the core, the light gradually fades into a more diffuse halo or envelope. While a definite disk structure is not apparent, there is a slight elongation visible, presenting an in-between roundness. No pronounced spiral arm features or dust lanes are discernible in this observation. Overall, the galaxy appears largely undisturbed, with no immediate evidence of a major merger event or significant tidal disruption. The color profile shows an apparent trend from g to r to z bands, meaning that the color appears to become slightly redder as you move from the g to r to z bands.
