The galaxy presents as a relatively faint, elongated structure with a major axis noticeably longer than its minor axis, suggesting a flattened, possibly disk-like morphology seen at an oblique angle. A dominant central bulge is not readily apparent, however, there is a bright point near the center which is likely the galactic center. There is a smooth light distribution which indicates that the galaxy is more likely an elliptical. There is little evidence of spiral arm structure or significant dust lanes. The color profile appears to be slightly redder in the central regions and blue closer to the edges, indicative of an older stellar population towards the center and younger stars in the periphery. There is no visible evidence of ongoing merger activity or tidal disturbances. The system appears generally undisturbed and isolated based on this image.
