The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. The light distribution appears largely uniform, suggesting a lack of significant spiral arms or prominent substructures. There is a subtle elongation, hinting at a slight deviation from perfect circularity, but overall it is fairly round in appearance.

The galaxy's color is skewed towards the green-red end of the spectrum. There are no obvious signs of recent or ongoing major merging events, such as tidal tails or strong asymmetries in the light profile. However, there seems to be a minor disturbance happening; subtle irregularities in the outer regions suggest possible interactions or a minor accretion event.
