The galaxy presents a relatively smooth morphology. There is a slight degree of asymmetry noticeable; possibly an ongoing minor interaction. The galaxy is somewhat elliptical but tends towards a more intermediate shape. A significant portion of light appears to originate from the central region, with a gradual decline in brightness outwards. Based on color index, the galaxy's stellar population indicates a moderately passive galaxy, with some regions of weak star formation still active. A possible tidal feature is present, lending evidence to a previous interaction or merger. There is no clear visual evidence of spiral arms or a prominent disk.