The galaxy presents a relatively smooth, concentrated appearance, suggestive of an elliptical morphology or a late-stage merger remnant. There is a distinct, centralized condensation, indicating a possible core or bulge region with a relatively high concentration of older stars. The overall color of the galaxy appears yellowish-orange, which would be consistent with a stellar population dominated by older, redder stars and a subdued rate of on-going star formation. The light distribution suggests a largely spheroidal shape, however it also presents itself with a subtle disturbance within its shape. There may be faint tidal features or shells present, but due to the image resolution, this is difficult to ascertain conclusively. There is not a strong indication of spiral arms or a prominent disk component. Overall, the features suggest that this system is in the process of merging or is a quiescent elliptical galaxy.
