This galaxy appears as a moderately bright, slightly elongated object. The light distribution is generally smooth, suggesting an elliptical morphology or a spiral galaxy viewed at a high inclination. The galaxy exhibits a color gradient, appearing bluer towards the outer regions and redder towards the center, potentially indicating a population of younger stars in the periphery and older stars concentrated in the bulge. There is a slight suggestion of faint, diffuse arms or tidal features. Overall, the galaxy appears relatively undisturbed, with no clear signs of a major ongoing merger, although the subtle asymmetries could indicate minor past interactions. The roundness of the object indicates that it is somewhere between perfectly round and cigar shaped. The light distribution suggests that the object is smooth rather than featured.
