The galaxy presents a primarily elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. There is a noticeable absence of distinct spiral arms or a prominent disk structure. The central region displays a high surface brightness, suggesting a dense stellar population, potentially indicative of a bulge component or a supermassive black hole at the core. The galaxy's color appears generally redder, implying an older stellar population with less ongoing star formation. The overall shape suggests a slightly elongated or flattened structure. There are no obvious signs of recent major mergers or tidal disturbances in its immediate vicinity. The galaxy appears relatively isolated, without any apparent companion galaxies undergoing interaction.
