The galaxy presents as a relatively smooth, elliptical morphology, with no apparent spiral arm structures or prominent dust lanes visible. Its overall color suggests a population of older stars, exhibiting a yellowish hue. The central bulge is well-defined, appearing brighter and more concentrated than the outer regions of the galaxy. There is a gradual decrease in luminosity from the core outwards, indicating a smooth distribution of stellar density. The galaxy appears largely undisturbed, with no obvious signs of ongoing major mergers or tidal interactions. The object is compact, with a discernible boundary, and classified as an elliptical galaxy.