The galaxy presents a largely smooth, elliptical morphology, showing a distinct central bulge. The light profile appears centrally concentrated with a gradual decrease in surface brightness towards the outer regions. There is little evidence of spiral arm structures or significant dust lanes. The overall color is relatively uniform, leaning towards the redder end of the spectrum, suggesting an older stellar population. Slight disturbances may be present in the outer halo, but these appear minor. The galaxy appears isolated, with no obvious signs of a recent major merger or strong tidal interaction.
