The galaxy presents a largely smooth and elliptical morphology. The light distribution appears centrally concentrated with a gradual decrease in surface brightness moving outwards. There is a subtle color gradient, with the core region exhibiting a yellowish-orange hue suggesting an older stellar population. The outer regions of the galaxy transition towards a slightly bluer color, potentially indicating the presence of some younger stars or ongoing, albeit subdued, star formation. There are no clear indications of prominent spiral arms or a well-defined disk structure. The overall appearance suggests that this is a relatively massive system with limited recent merger activity or major disturbances. The shape is almost perfectly round, indicating a low degree of ellipticity. There is a slight asymmetry in the faint outer regions.
