This galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is elliptical, appearing nearly circular. The light distribution shows a strong central bulge that transitions gradually into a fainter, more diffuse halo. The color profile indicates a redder core, possibly suggesting an older stellar population. The outer regions exhibit a bluer tinge, which may indicate the presence of some younger stars or ongoing star formation. There are no apparent spiral arms or significant dust lanes visible in this image. The galaxy exhibits a weak hint of a disturbance in its outer edges, but overall appears unperturbed.
