The galaxy presents as a fairly symmetrical, centrally concentrated object with a smooth, diffuse appearance. A bright, yellowish core region transitions gradually into a more extended halo of bluer light, suggesting ongoing or recent star formation in the outer regions, with a population of older, redder stars dominating the core. There's a subtle elongation visible, deviating slightly from a perfectly circular shape, but no strong evidence of distinct spiral arms or a bar. The galaxy appears relatively undisturbed, showing no obvious signs of major mergers or tidal interactions. Faint ripples or shells might be present in the outer halo, requiring further investigation. The color gradient from the core to the outer regions indicates a radial variation in stellar populations and star formation activity. The estimated size of this galaxy is relatively small and is classified as an elliptical galaxy.
