The galaxy presents a generally elliptical morphology, though a disk structure is suggested by the image. The color distribution appears heterogeneous, with a concentrated, brighter yellowish-white central bulge or core, possibly indicating a population of older stars. Extending outward from the central region, fainter, bluish-white regions are observed. This bluer color potentially signifies the presence of younger, hotter stars and ongoing star formation within the disk. No spiral arm structures are clearly visible, and the galaxy appears relatively undisturbed. The light distribution suggests the galaxy is moderately inclined with respect to our line of sight. The overall structure indicates a system of significant mass and moderate star formation activity.
