The galaxy presents as a centrally concentrated object, exhibiting a predominantly smooth morphology. The core is well-defined and emits strongly in green wavelengths, which is consistent with observations done through DESI. There is a notable absence of clearly defined spiral arm structures or prominent dust lanes.

The overall shape appears to be close to circular, with only slight deviations from perfect roundness. No strong tidal features, such as tails or bridges, are discernible, suggesting a relatively undisturbed state, although subtle asymmetry cannot be ruled out entirely. The galaxy seems to be isolated and not obviously interacting with any nearby galaxies, but close inspection shows very minor disturbances.
