The galaxy presents a generally smooth morphology, exhibiting a dominant elliptical shape. The light distribution appears concentrated towards the center, indicating a prominent bulge. The galaxy shows a slight deviation from perfect roundness, leaning towards a moderately elliptical form. There are no clear signs of spiral arm structures or significant dust lanes. The overall appearance suggests a relatively evolved system, likely with an older stellar population. No major merging events or significant tidal disturbances are readily apparent in the image.
