The galaxy presents a generally smooth and elliptical morphology, with a high degree of central concentration. The overall shape appears to be somewhere between round and cigar-shaped. The central region exhibits a bright, yellowish hue, suggesting a population of older stars. This core is surrounded by a less concentrated, slightly bluer halo. There is some minor color variation within the halo, indicating subtle differences in stellar populations. No prominent spiral arms or distinct dust lanes are apparent. There is no immediately obvious indication of any major ongoing merger activity or strong tidal disturbances, though there are hints of some minor disturbances in the halo. Overall, the galaxy appears to be relatively quiescent and evolved, with a significant stellar mass and low ongoing star formation.
