The galaxy exhibits an elliptical morphology, though there is some potential distortion suggestive of a disk-like structure when viewed from a slight angle. The central bulge is well-defined and possesses a concentrated, luminous core, appearing a yellowish-white hue. This color likely indicates an older stellar population. 

Surrounding the bulge is a more diffuse halo, showing hints of bluer regions. These suggest the presence of younger, hotter stars potentially involved in recent or ongoing star formation. The outer regions are less defined, fading into the background sky with no obvious tidal features or signs of major ongoing mergers. However, there may be minor disturbances present, given the slightly irregular shape of the outer halo. The overall color gradient transitions from the yellow-white core to the bluer outer regions. The galaxy appears relatively isolated, without any other significant galaxies in its immediate vicinity to suggest interactions.
