The galaxy presents as a centrally concentrated, lenticular-like structure. Its morphology appears to be dominated by a relatively smooth, diffuse light profile. The core region exhibits a high degree of luminosity, transitioning into a fainter, more extended halo. Evidence of asymmetry is present, with a potential minor disturbance or interaction visible within the disk. There is a luminous clump within the disk that may indicate star formation. Overall, the galaxy appears to be in a transitional phase, possibly evolving towards a more spheroid-dominated morphology.
