The galaxy presents as a somewhat featureless, elliptical morphology. Its shape is moderately elongated, appearing more cigar-shaped than circular. The galaxy appears to be relatively smooth with a bright central bulge that shows a slight blue hue. There is no clear evidence of spiral arms or significant dust lanes. Faint color variations are observable, primarily in the central region, with a possible hint of younger, bluer stars towards the center and redder populations in the outer regions. This is consistent with an older stellar population, likely with ongoing, but reduced, star formation. The galaxy does not appear to be undergoing any major merging events or tidal disturbances, though a minor disturbance cannot be ruled out. The overall structure suggests a relatively evolved system.
