The galaxy appears as a relatively compact, centrally concentrated object. The overall structure presents a smooth morphology with minimal discernible features such as spiral arms or a prominent disk. The light distribution suggests an elliptical or lenticular galaxy type. The central region exhibits a slightly brighter concentration of light, suggesting the presence of a galactic nucleus or a bulge. There is a subtle elongation or asymmetry to the overall shape, possibly indicating minor tidal disturbances or interactions with another galaxy, though no clear merging signatures are observed. The color appears relatively uniform, with a possible slight redder hue, indicating a potential population of older stars.
