The galaxy appears as a centrally concentrated, elliptical-like structure. It is primarily a smooth, featureless object, lacking any obvious spiral arms or a prominent disk component, with a smooth bulge-like structure. There may be a slight elongation, suggesting it is somewhat aspherical. The galaxy exhibits a color gradient, with a slightly yellower or redder central region, suggesting an older stellar population in the core, and bluer outskirts which are indicative of younger stars. There is no evidence of any significant tidal disturbances or ongoing major mergers with other galaxies. The galaxy appears to be an isolated elliptical galaxy undergoing limited star formation.