The galaxy presents as a centrally concentrated object, exhibiting a generally smooth morphology. There is little to no indication of spiral arm structure, or patchy regions of star formation. The galaxy's light profile appears relatively uniform, diminishing gradually from a bright central core. The shape is generally round, with a hint of elongation along one axis. There is no obvious indication of ongoing major merger activity, tidal tails, or strong morphological distortions. The color profile appears generally consistent across the galaxy, trending towards redder wavelengths.
