The galaxy presents as a moderately luminous, relatively compact object with a redshift of z ≈ 0.145. It exhibits a bright, somewhat concentrated central region that transitions into a fainter, more diffuse halo. The shape is approximately elliptical but shows some signs of asymmetry, leaning towards a disc shape, suggesting a possible early-type spiral or lenticular galaxy. There is a slight bluish tint in the outer regions, which may indicate some ongoing, albeit limited, star formation. There are no apparent signs of a major merger event, however, there is a very subtle asymmetry that indicates either a very minor merger or tidal disturbances in the galaxy. Overall, the galaxy appears to be in a relatively evolved state, possibly transitioning from a spiral to an elliptical morphology.
