The galaxy appears to be a relatively smooth, elliptical-like system with a concentrated central bulge. There is a noticeable radial color gradient, transitioning from a yellowish-white core to a redder outer halo. The overall shape is generally round, though there are possible subtle deviations that may indicate a slight elongation. No distinct spiral arm structures or dust lanes are visible. The galaxy appears relatively isolated, showing no strong signs of ongoing major mergers or significant tidal disturbances, though a slight asymmetry in its morphology could indicate minor interactions in its past or present.
