The galaxy appears as a single, relatively smooth, concentrated light source. The color is predominantly yellowish-orange, suggesting an older stellar population with fewer hot, young blue stars. There is little evidence of spiral arms or significant dust lanes. It has an elliptical-like structure. There may be a hint of a very faint, extended halo surrounding the central region, but this is not well-defined. The galaxy does not seem to be currently undergoing any major merging events or exhibiting strong tidal disturbances. Overall, it appears to be a galaxy with a fairly regular, relaxed morphology.
