The galaxy presents as a relatively smooth, elliptical morphology. The core exhibits a bright, concentrated luminosity, with a gradual decrease in surface brightness extending outwards. There is little evidence of spiral arm structure or significant dust lanes. The overall color appears to be dominated by redder wavelengths, possibly indicating an older stellar population and/or the presence of dust, though not visually prominent. Faint, blue-ish features are visible surrounding the brighter, redder core, potentially indicating ongoing star formation, though appearing at a relatively low rate. There are no obvious signs of a major merger or strong tidal distortions, though a subtle asymmetry in the outer halo cannot be ruled out.
