This galaxy appears to be a relatively smooth, elliptical galaxy, with a highly concentrated central bulge. It exhibits a near-spherical shape, showing minimal deviation from roundness. There's no obvious evidence of spiral arm structure or a prominent disk component. The galaxy displays a smooth light profile, gradually decreasing in brightness from the center outwards, suggesting a fairly homogeneous stellar population. No major merger or tidal disturbance is apparent in the image. The central region has a yellowish-white hue, possibly indicating a population of older, evolved stars. The galaxy's outer regions show hints of bluer colors, potentially caused by low level star formation activity or the presence of younger stars.
