The galaxy presents a generally smooth, elliptical morphology, with an apparent roundness leaning towards the oblate spheroid classification. Its color profile suggests a primarily older stellar population. There is a clear concentration of luminosity towards the galactic nucleus, indicating a possible supermassive black hole actively drawing matter. The disk exhibits a relatively low level of star formation. There does not appear to be any ongoing major mergers with another galaxy and the morphology of the spiral disk seems to be undisturbed, indicating that there is nothing interacting with it. This supports the idea that the galaxy does not appear to be interacting or disturbed by external forces.
