The galaxy presents an elliptical morphology, with a noticeable bulge. The light profile suggests a smooth distribution, indicative of an older stellar population, although some bluer regions exist throughout the galaxy, likely pockets of younger stars. The galaxy appears relatively compact, exhibiting a high degree of central concentration. The overall color is somewhat redder with a yellowish-white appearance in the center, consistent with a galaxy whose star formation is in decline. The angle of the galaxy is not face on, and is slightly inclined. It does not show any obvious signs of active galactic nuclei or strong tidal disturbances.
