The galaxy presents as an elliptical morphology, exhibiting a generally smooth light distribution. The central region appears brighter and more concentrated, showing a yellowish hue suggesting an older stellar population. Moving outwards from the core, the color subtly shifts to a slightly bluer tinge, indicating the presence of younger stars, though the overall color remains relatively consistent. There is no discernible spiral arm structure or significant dust lane obscuration apparent in this image. The galaxy appears relatively isolated, with no obvious signs of a major ongoing merger or tidal disturbances. The observed shape is moderately elliptical, tending towards roundness. A minor asymmetry may be present, but further investigation is required to confirm.
