The galaxy appears to be a relatively smooth, elliptical type. Its light is concentrated towards the center, forming a bright, yellowish core. The galaxy's shape is largely circular, with only a slight deviation towards an oblong form. There is no discernible spiral structure or prominent dust lanes. Faint extensions of light are visible around the central region, suggesting a diffuse halo. The overall color is dominated by older stellar populations, indicating a lower rate of ongoing star formation. There is no obvious evidence of recent or ongoing merger activity or significant tidal disturbances in the galaxy's structure.
