The galaxy presents as a moderately bright, somewhat diffuse object. Its morphology appears largely smooth, with a suggestion of a flattened, though not strongly defined, shape. The light distribution exhibits a central concentration, fading towards the edges. There is no clear evidence of spiral arm structure or a prominent disk. The color profile suggests an intermediate stellar population, neither strongly blue, indicative of active star formation, nor overtly red, signaling an older, quiescent population. There are no signs of significant disturbances or tidal features that would indicate recent mergers or interactions. The overall appearance points towards a galaxy that is relatively evolved and stable.
