The galaxy presents as a centrally concentrated spheroid with a smooth overall light distribution. There is a distinct, bright core region which fades gradually towards the outer regions. A subtle bluish tinge dominates the central region, suggesting the presence of younger, hotter stars. The shape appears to be generally elliptical, without strong evidence of spiral arm structure or significant dust lanes. There is a lack of any obvious signs of tidal disturbances or ongoing major mergers, suggesting a relatively undisturbed morphological state. The galaxy seems to be a fairly evolved system.
