The galaxy presents as an elliptical or lenticular system, exhibiting a generally smooth morphology with no readily apparent spiral arm structures. Its shape appears to be somewhere between round and elongated. The galaxy's core is a bright, concentrated region, suggesting a high density of stars. There are no obvious signs of major mergers or significant tidal disturbances. However, there is potentially some minor irregularity that could be interpreted as a minor disturbance. The stellar population appears relatively old with low star formation.
