The galaxy presents as a slightly elongated, lenticular form with a prominent central bulge. A notable feature is the distinct color gradient observed across the galaxy. The core appears to be dominated by bluish-white light, suggestive of a population of hotter, younger stars. Moving outward from the core, there's a transition toward a redder hue, particularly noticeable on one edge of the disk. This suggests the presence of older stellar populations or dust obscuration in these regions. The galaxy exhibits a relatively smooth appearance, with only subtle indications of spiral arm structure. The overall morphology suggests a relatively evolved system, perhaps undergoing or having recently undergone significant star formation activity. There is also a slight visual disturbance on one side of the galaxy, which could be from a minor merger.
