The galaxy presents a primarily smooth morphology, with an approximate effective radius of 8.3 kiloparsecs. It displays a slight disklike appearance with a central bulge, although spiral arms are not distinctly visible. The galaxy appears to be relatively isolated, with no obvious signs of major mergers or significant tidal disturbances. There may be some indication of minor disturbances. The central region exhibits a yellowish color, suggesting an older stellar population, while the outer regions have bluer tones, which could potentially indicate ongoing or recent star formation. The overall shape could be described as moderately rounded, appearing neither perfectly spherical nor highly elongated. The estimated stellar mass appears substantial, suggesting a mature system.
