The galaxy appears as a centrally concentrated object with a generally smooth morphology. Its shape is approximately round. The central region exhibits a relatively brighter concentration of light, suggestive of a bulge. Faint, diffuse light extends outwards from the core. The color appears to be somewhat blueish, hinting at the presence of younger stellar populations. There are no obvious signs of spiral arm structure or major disturbances. The galaxy shows no clear evidence of being involved in a major merger, though some subtle asymmetry might imply minor interactions. Overall, the galaxy's characteristics lean towards being an elliptical or lenticular type galaxy. It exhibits a low rate of star formation.
