The galaxy presents as a centrally concentrated, relatively smooth object.  It exhibits a rounded morphology, with a gradual decrease in luminosity from the core outwards. The central region is bright and diffuse, showing a dominance of older stellar populations which contribute to its redder color.  There is little to no evidence of distinct spiral arm structures or prominent dust lanes.  The faint outer regions suggest a halo component, but it is not well defined in this image.  There might be some minor asymmetry within the halo, suggestive of tidal interactions but is difficult to conclude.  Overall, the galaxy appears to be an evolved system.
