The galaxy presents as a slightly elongated structure with a discernible central bulge that appears yellowish-white in color, indicating a population of older stars. There's evidence of a faint, diffuse disk component that may extend from the bulge. The galaxy exhibits a degree of asymmetry, possibly a sign of past or ongoing interactions. A faint, diffuse greenish patch exists near the main body of the galaxy, potentially indicative of some ongoing star formation, though the overall star formation rate appears relatively low. The galaxy exhibits a generally smooth appearance, suggesting that it is an evolved system.
