The galaxy presents a generally smooth, elliptical morphology with no obvious spiral arm structure. It exhibits a concentrated central bulge that appears yellowish-white, suggesting a population of older stars. The galaxy's overall color profile is relatively uniform, with subtle color gradients indicating a possible change in stellar population density moving outward from the center. Based on the light profile, the galaxy is likely a relatively quiescent system with a moderate stellar mass and low ongoing star formation. No significant tidal features or signs of recent mergers are apparent in the immediate vicinity of the galaxy. The galaxy’s overall appearance points toward a more evolved stellar population.
