The galaxy presents a generally smooth and concentrated morphology. The central bulge is prominent, exhibiting a bright, yellowish-orange hue. Surrounding the bulge is a more diffuse, greenish halo. There are hints of faint, spiral-like structures or tidal disturbances emanating from the central region, but they are not sharply defined. The overall shape appears somewhat round, though subtle deviations suggest it may be slightly elongated. While no major merger events are apparent, there are subtle asymmetries that indicate possible past minor disturbances. There is evidence of ongoing, but relatively low, star formation activity. The galaxy exhibits substantial mass.
