The galaxy presents a somewhat amorphous morphology, appearing neither purely elliptical nor distinctly spiral.  There is a subtle elongation, suggesting a departure from perfect sphericity. The light profile appears relatively smooth, with a dominant central concentration. Patches of bluer color can be observed, interspersed throughout the galaxy, which may be indicative of regions of active star formation. A more pronounced redder region is noticeable at one edge of the galaxy. Overall, the galaxy exhibits a moderate degree of disturbance. The galaxy has a substantial mass and a modest star formation rate.
