This galaxy presents a largely smooth morphology with a central bulge that appears to be roughly elliptical in shape. The light distribution is concentrated towards the center, indicating a possible dominance of older stellar populations. The galaxy exhibits an intermediate roundness, appearing neither perfectly spherical nor highly elongated. There are no prominent spiral arms, bars, or other significant features suggesting a disk structure. A small portion on the right of the galaxy may have more star formation. There is no obvious evidence of ongoing mergers or tidal disturbances. Overall, the galaxy appears to be a relatively undisturbed system.
