The galaxy appears as a relatively smooth, centrally concentrated object. Its morphology seems largely elliptical, presenting a fairly regular and rounded structure without prominent spiral arms or a distinct disk-like appearance. There are no obvious signs of ongoing merging activity or major disturbances in its overall shape, although there appears to be a slight distortion in the structure. The galaxy exhibits a strong concentration of light towards its core, with the light appearing slightly yellow-reddish, possibly indicating an older stellar population and a lower rate of star formation. The galaxy is moderately sized.