The galaxy presents as a single, fairly smooth object with a concentration of light towards its center, suggesting a bulge. There is faint evidence of a possible disk component, but the overall structure is relatively featureless. The galaxy's light distribution appears mostly spheroidal, with a slight elongation. It has an orange-red hue, indicating an older stellar population and/or significant dust content. There is little to no evidence of spiral arms or other distinct features within the galaxy's disk, although some patchy regions are present that might have some star formation, but it may also be due to image artifacts. There are no obvious signs of a major ongoing merger or strong tidal disruption. There is no dust lane evident, but a redder center suggests some level of dust obscuration in the galactic nucleus.
