The object appears to be a relatively smooth galaxy, exhibiting a generally elliptical morphology. Its light is concentrated towards the center, with a gradual falloff in surface brightness with increasing radius. There's little evidence of distinct spiral arm structures. The galaxy appears relatively undisturbed, with no major signs of ongoing mergers or tidal interactions. The light distribution indicates an evolved stellar population, consistent with a relatively high degree of central concentration. The roundness is apparent, with the galaxy's major and minor axes being of similar length. There may be slight disturbances or asymmetries in the outer regions of the galaxy but it is unlikely to be a major disturbance.
