The galaxy presents as an elliptical or lenticular type with a smooth, centralized light distribution. There is little to no evidence of spiral arms or a distinct disk component, although the image resolution is limited. The galaxy appears largely featureless, with no obvious dust lanes, star-forming regions, or tidal tails indicating recent mergers or interactions. The light profile is concentrated towards the center, with a gradual falloff in intensity outwards. The color appears somewhat yellow, suggesting an older stellar population with relatively little ongoing star formation. Its apparent roundness suggests that it is either intrinsically spherical or viewed face-on. There appears to be no major disturbance visible.
