The galaxy presents a predominantly smooth morphology. There is a slight central concentration of light, appearing nearly spherical and slightly elongated along the horizontal axis. A subtle disk-like structure might be present within the central region; however, the smoothness of the galaxy overall suggests it is likely an elliptical galaxy. No prominent spiral arms or bars are discernible. The color profile suggests a population of older stars. There may be an active galactic nucleus. There is no evidence of any tidal tails or merging features that indicate recent major interactions, but a subtle asymmetry cannot be ruled out. Star formation is likely occurring, but at a low rate.