The galaxy appears to be a relatively smooth, elliptical-like structure with a bright, concentrated central bulge. There is a gradual fading of light intensity moving outwards from the core to the outer regions, suggesting a decreasing stellar density. The color profile indicates a generally older stellar population, especially in the central bulge, with a yellow-red hue dominating. There's some evidence of bluer light in the outer regions, potentially indicating pockets of younger stars or ongoing star formation, but these are subtle. The overall morphology lacks any clear spiral arm structure or significant dust lanes. The galaxy exhibits a moderate level of roundness, appearing neither perfectly spherical nor highly elongated. There are no obvious signs of major mergers or significant tidal disturbances affecting the system.
