The galaxy presents as an elliptical or lenticular type, exhibiting a largely smooth and featureless morphology. The light is concentrated towards the center, suggesting a prominent bulge component. A slight elongation is visible, though the galaxy is generally round. There is no discernible spiral arm structure or bar present. The color profile suggests a relatively evolved stellar population with a moderate level of on-going star formation, evidenced by the presence of some bluer regions. There appears to be minimal interaction or disturbance from neighboring galaxies.
