The galaxy presents as a concentrated, luminous central bulge, surrounded by a fainter, more diffuse disk. The bulge exhibits a smooth, relatively featureless morphology. The disk appears to be inclined at a substantial angle relative to our line of sight. Some subtle irregular features are visible, particularly in the disk, suggesting potential minor disturbances, though no large scale tidal features can be identified. The color gradient indicates older stellar populations concentrated in the bulge. Traces of bluer color in the disk might be indicative of ongoing star formation. The overall shape leans toward an elliptical form, yet there exists evidence supporting a disk structure, placing it somewhere between a pure elliptical and a spiral galaxy.
