The galaxy presents as an elliptical morphology. The object appears largely smooth with a notable central bulge exhibiting a concentrated luminosity gradient. The color profile suggests an older stellar population, with a dominant red/yellow hue emanating from the core, transitioning to a slightly bluer halo on its periphery. There is no obvious indication of spiral arm structure or prominent dust lanes. The galaxy is slightly elongated. No signs of tidal disturbances or active galactic nuclei activity are evident. Based on its integrated light profile, the galaxy is potentially undergoing a low rate of star formation.
