The galaxy presents as an elliptical structure with a bright, concentrated central bulge that dominates its overall luminosity. The light distribution appears smooth, indicative of an older stellar population. The disk is quite face-on, with some evidence of a minor warp or tilt. The outer regions are fainter but appear well-defined, suggesting a relatively sharp cutoff in stellar density. There is some subtle mottling throughout the disk that could be due to faint dust lanes or patches of star formation, though this is difficult to discern due to the image quality. The elongation of the galaxy suggests an oblate spheroid shape, and the position angle of the major axis is approximately Northwest to Southeast. There is no sign of strong tidal features or recent merger activity.
