The galaxy presents a largely smooth, elliptical morphology. There is a highly concentrated central bulge exhibiting a yellow-gold hue, indicative of an older stellar population. This bulge region appears to dominate the light output. Surrounding the core is a less concentrated disk. This outer region displays a blueish tint, hinting at a younger, hotter stellar population with ongoing star formation. The overall structure appears relatively undisturbed, with no major signs of tidal interactions or ongoing mergers, though a degree of asymmetry suggests minor disturbances may be present. The shape is generally round, but with some evidence of elongation. There are no visible spiral arms or bar structures.
