The galaxy presents as a relatively smooth, centrally concentrated elliptical or lenticular form. The light distribution appears centrally peaked, with a gradual decrease in intensity moving outward from the core. The central region exhibits a yellowish hue, suggesting an older stellar population.  There appears to be little or no evidence of spiral arm structure or significant dust lanes.  The overall shape seems to be tending more towards roundness, than a highly elongated shape. There is no visible evidence of tidal tails, strong interactions, or other significant morphological disturbances.
