The galaxy presents as a single, relatively smooth object with a concentrated central region. There is little to no discernible structure such as spiral arms or a bar. The light distribution appears fairly uniform, with a gradual decrease in brightness moving outwards from the core. The color profile indicates a general yellowish-white hue, suggesting an older stellar population with fewer hot, young stars. There is no indication of any major ongoing mergers or significant tidal disturbances. The galaxy exhibits a generally round shape with only a slight deviation from perfect circularity. The overall impression is of a relatively quiescent system.
