The galaxy appears to be a relatively compact elliptical. It presents a smooth, centrally concentrated luminosity profile, with no obvious spiral arms or a distinct disk structure. The galaxy exhibits a color gradient, with a yellowish-white core that transitions to a slightly redder halo. This color gradient suggests a population of older stars dominating the central region, and a potentially younger, more metal-poor stellar population further out. No signs of significant dust lanes, star-forming regions, or tidal disturbances are evident. The morphology indicates that the galaxy is undisturbed and likely quiescent in terms of star formation. It is round, and shows no signs of recent mergers or interactions.
