The galaxy presents an elliptical morphology, appearing largely smooth and featureless. The central bulge exhibits a bright, concentrated luminosity, suggesting a high density of stars. The color profile indicates a dominance of older stellar populations, with a general lack of blue light indicative of recent star formation. It appears mildly elongated, but is mostly round. There is no clear evidence of spiral arm structure or active galactic nuclei. No signs of tidal tails or significant distortions are visible, suggesting the galaxy has not undergone a recent major merger event.
