The galaxy presents a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that dominates the overall luminosity. The light distribution appears to decline smoothly from the center outwards, without prominent spiral arms or other distinct features. The galaxy's color index suggests the presence of a primarily older stellar population, with a lower rate of current star formation activity. There is a slight deviation from a perfectly circular shape; it appears more 'in-between' rounded. No major disturbances or signs of ongoing mergers are readily apparent. The overall impression is that of a quiescent, relatively evolved galaxy.
