The galaxy presents an elliptical morphology, appearing largely featureless and smooth in texture. Its core exhibits a concentrated, bright luminosity, suggesting a dense stellar population or possible AGN activity. The light gradually diffuses outward from the core, indicating a decreasing stellar density with radial distance. The galaxy appears slightly elongated, showing a shape somewhere between round and cigar-shaped. There are no obvious signs of spiral arms or a prominent disk structure. No major mergers or significant tidal disturbances are immediately evident. A faint, diffuse structure is present around the main body, possibly indicating a stellar halo or extended galactic envelope. The galaxy displays a reddish-yellow hue, which suggests a population of older, cooler stars and/or dust obscuration. A small, adjacent galaxy or star cluster is present to the side of the main galaxy.
