The galaxy appears to be an elliptical galaxy, exhibiting a smooth, spheroidal morphology with little discernible structure. The light distribution suggests a centrally concentrated bulge, characterized by a yellowish hue, indicative of an older stellar population. Fainter, bluer light is diffused around the core, possibly indicative of some younger stars, or low levels of recent star formation. There is no evidence of a disk component or spiral arms. The galaxy appears relatively undisturbed, with no clear signs of a major merger or significant tidal interactions, although there is some hint of minor disturbance. Overall, the galaxy's morphology suggests it is a relatively massive system that is approaching quiescence.
