The galaxy appears to be a relatively smooth, disk-dominated system. Its overall morphology suggests an elliptical shape with a notable bulge component. The central region exhibits a yellow-orange hue, potentially indicative of an older stellar population. Moving outwards from the core, a faint blue-greenish disk is visible, suggesting the presence of some younger stars or ongoing star formation. There may be a slight asymmetry or subtle distortions in the outer disk, though no major mergers or tidal features are immediately obvious. The galaxy is neither perfectly spherical nor highly elongated, falling somewhere in between.
