The galaxy presents as a single, largely homogenous body with a slightly elliptical shape, approximating a spheroid. A central bright region indicates a possible galactic nucleus, although this is not distinctly resolved. The galaxy exhibits a smooth, diffuse structure with a dominant blue hue, suggesting a population of younger, hotter stars. There is no apparent spiral arm structure or dust lane features visible. Given the overall morphology, the galaxy is likely an elliptical, with a high degree of radial symmetry and no apparent ongoing major mergers or tidal interactions. Minor disturbances, while not pronounced, cannot be entirely ruled out. The overall colour suggests relatively moderate levels of star formation are likely occurring.
