The galaxy appears as a somewhat elliptical, luminous object. The light is concentrated in the center, with intensity gradually decreasing outwards. A color gradient is observed, with the central region exhibiting a yellowish-white hue, suggesting an older stellar population. The outer regions appear slightly redder, potentially indicating the presence of dust or cooler stars. The overall structure seems largely smooth, with little evidence of spiral arms or irregular features. The morphology is consistent with that of an elliptical galaxy, possibly of intermediate ellipticity. Faint extensions might be present, but they are difficult to resolve with the current image resolution. There may be a subtle asymmetry, or minor tidal disturbance, hinting at past interactions, but it is not highly pronounced.
