The galaxy presents as a somewhat elongated spheroid, appearing mostly smooth in texture. Its color profile consists of a central, bright, concentrated region exhibiting a white to slightly yellow hue. This likely indicates a concentration of older stellar populations within the galactic nucleus. Moving outwards from the core, the light transitions to a blueish color. The periphery lacks defined spiral arm structures, suggesting either a relatively quiescent star formation rate or a galaxy type other than a grand design spiral. The overall shape indicates a possible elliptical galaxy or a lenticular galaxy viewed at an angle. There is a slight asymmetry to the outer edges, suggesting a possible minor interaction or disturbance in its recent past. There is no clear evidence of tidal tails or strong distortions associated with major merger events. The angular size is relatively small.
