The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is little evidence of prominent spiral arms or dust lanes. The galaxy exhibits a color gradient, transitioning from a yellowish-white core to a fainter, bluish halo. This color gradient suggests the presence of older stellar populations concentrated towards the center, with younger, bluer stars more dispersed in the outer regions. The galaxy appears generally undisturbed, showing no obvious signs of ongoing major mergers or significant tidal interactions. There may be some indication of minor disturbances in the outskirts, but this requires further investigation. The overall morphology points towards an evolved system, likely undergoing relatively low levels of star formation.
