The galaxy presents as a relatively smooth, elliptical morphology. It appears to be a mature system, evidenced by the predominantly yellowish-white color profile suggesting an older stellar population with less ongoing star formation. No distinct spiral arms or prominent dust lanes are discernible. The galaxy exhibits a high degree of central concentration with a gradual decrease in luminosity moving outwards from the core. The shape appears mostly round, though with some slight elongation. There are no obvious signs of recent or ongoing major mergers or tidal disturbances.
