The galaxy presents as an elliptical morphology, elongated with a high degree of ellipticity. A central bulge is visible, exhibiting a bright, concentrated core that fades into a more diffuse halo. There's a lack of any discernible spiral arm structure or prominent dust lanes. The overall color appears to be a relatively uniform bluish-white, suggestive of a moderate population of younger, hotter stars alongside an older stellar population. The smoothness of its light distribution indicates that the galaxy has likely undergone significant dynamical relaxation, with minimal signs of recent major mergers or tidal disturbances. Some faint features or shells could potentially be present, but are not easily visible within the image's resolution and contrast.
