The galaxy presents as a relatively smooth, concentrated object with an overall elliptical morphology. The central region is a bright, yellowish-gold, suggesting a dominant population of older stars. The galaxy displays a gradual decrease in luminosity from the core outwards. There appears to be a slight disk-like structure, with hints of spiral arms, but they are not sharply defined. There is a faint blue region on one side of the galaxy, indicative of some ongoing star formation. The absence of strong tidal features suggests that the galaxy has not experienced a major merger recently, however there is some minor disturbance in the outer edges of the galaxy's shape. The galaxy is estimated to be 9.23 kpc in radius, with no clear signs of dust lanes or significant obscuration.
