The galaxy presents as a relatively smooth, centrally concentrated object with an elliptical morphology. A bright central bulge is apparent, surrounded by a fainter, more diffuse halo.  The light distribution suggests a lack of significant spiral arm structure, although subtle variations in color across the galaxy body might indicate underlying structures.  There appears to be little to no evidence of major mergers or significant tidal disturbances. Overall, the galaxy exhibits a somewhat rounded, non-elongated form. The integrated color indices suggest moderate star formation may be present, but not at a particularly intense rate.
