The galaxy appears to be a relatively compact, elliptical or lenticular galaxy, exhibiting a generally smooth and symmetrical morphology. The color profile suggests an older stellar population, with a concentration of yellow and red light towards the core, indicative of evolved stars. There is little evidence of ongoing or recent star formation, as indicated by the absence of distinct blue or irregular features. The galaxy appears quite round in shape, lacking any significant elongation or bar structure. There is no readily apparent evidence of tidal disturbances or ongoing mergers, however, there is some subtle asymmetry in the outer regions, suggesting a possible minor interaction in the past.
