The galaxy presents as a relatively smooth, elliptical-like structure. The core is a concentrated, bright yellowish-white, suggesting an older stellar population with minimal ongoing star formation. Moving outward from the center, the color transitions to a reddish hue, implying a further dominance of older, redder stars. There is a lack of significant dust lanes or spiral arm structures. The galaxy appears largely undisturbed, with no signs of major mergers or tidal interactions. The morphology indicates a high degree of central concentration with a relatively compact structure.
