The galaxy presents an elliptical morphology, appearing relatively smooth and undisturbed. Its shape is somewhat elongated, exhibiting an axis ratio that leans towards an intermediate classification. The galaxy's core is characterized by a bright, concentrated nucleus, which gradually diminishes in luminosity toward the outer regions. There is a color gradient noticeable from the center outwards, with the core displaying a yellowish hue and the outer disk a bluer tint. This potentially indicates a central concentration of older stellar populations, with younger, bluer stars populating the periphery. There is no evidence of any major merging activity or significant tidal disturbances. The object appears to be an isolated system.
