The galaxy presents as a relatively smooth, round structure. There is a bright central bulge with a gradual decrease in luminosity towards the outer edges. The overall color appears slightly redder, potentially indicating an older stellar population. No distinct spiral arms or dust lanes are readily apparent. The galaxy exhibits a compact morphology, with a lack of extended features or tidal disturbances, and no signs of a major merger event. There might be a hint of disk structure present, but it is very faint. Overall, the galaxy appears to be an elliptical or S0 type, with little evidence of active star formation.
