The galaxy presents as a relatively smooth, centrally concentrated object. There is a gradual increase in luminosity towards the core, which appears bright and somewhat spherical. The outer regions display a fainter, more diffuse halo. It appears the galaxy is neither strongly elliptical nor a spiral. There is a lack of any obvious spiral arm structure or a distinct galactic bar within this galaxy. The overall morphology suggests a relatively evolved system with a significant spheroidal component. There are no readily apparent signs of any major mergers or significant tidal disturbances. The object's structure is suggestive of a possible early-type disk or elliptical galaxy with some star formation occurring.
