The galaxy presents a largely smooth and rounded morphology. It exhibits a dominant central bulge with a concentrated, bright core, suggesting a high density of stars. The color profile appears slightly redder, potentially indicating an older stellar population and lower levels of on-going star formation. No distinct spiral arm structures or significant dust lanes are visible. There is a subtle color gradient from the inner regions outwards. The overall appearance suggests an elliptical or lenticular galaxy type. There's no visual evidence of any major mergers or tidal disturbances impacting its structure.
