The galaxy presents an elliptical morphology, displaying a smooth light distribution that suggests an older stellar population. There is a lack of pronounced spiral arm structure. The central bulge is bright and concentrated, exhibiting a yellowish hue which indicates the presence of evolved stars. The outer regions of the galaxy appear less defined and fainter than the central bulge. The galaxy's overall color is slightly redder than that of a typical spiral galaxy, indicative of lower rates of star formation. There may be some indications of tidal interactions, but they appear minor in nature.
