The galaxy presents a largely smooth, elliptical morphology, with a high degree of central concentration. It exhibits a generally spheroidal shape, appearing almost circular, with only a slight suggestion of elongation. The light distribution appears very diffuse, with no distinct spiral arm features or prominent dust lanes visible. There is a suggestion of subtle color variation, with a yellowish hue concentrated in the core, possibly indicating an older stellar population. Fainter blueish tints extend outwards from the center. The galaxy appears relatively isolated, with no obvious signs of recent or ongoing major mergers or tidal disturbances. There might be very minor irregularities in the outer regions, possibly due to minor interactions.
