The galaxy presents as a somewhat flattened spheroid, exhibiting a smooth, elliptical morphology. There is a concentrated central bulge, noticeably brighter than the surrounding disk. The light profile appears relatively uniform, with no distinct spiral arm structures readily apparent. The galaxy displays a blueish hue, suggesting the presence of younger, hotter stars. The overall impression is that of a galaxy undergoing active, recent star formation. Faint disturbances may be present in the outer regions, hinting at past or ongoing interactions with other galaxies. The galaxy is neither perfectly circular nor highly elongated, but rather, occupies an intermediate shape. There is a hint of asymmetry but it could be due to artifacts.