The galaxy presents as a somewhat elliptical object with a smooth, centralized concentration of light. It exhibits a morphology leaning towards roundness, though there is a slight elongation, hinting at a shape somewhere between perfectly spherical and cigar-like. The galaxy’s overall appearance suggests a relatively evolved system with a dominant, older stellar population. There is no immediately obvious presence of distinct spiral arms or prominent dust lanes, instead light is rather uniform. There are no clear signs of ongoing major merging activity or significant tidal disturbances. Faint hints of a more disturbed structure could be present upon closer investigation, but this is not immediately apparent. Based on the color, there are no apparent signs of high rates of recent star formation.
