The galaxy presents a largely smooth morphology, appearing as a concentrated luminosity profile with a central bright region. The overall shape is somewhat elliptical, displaying a modest deviation from perfect circularity. There is a subtle indication of minor disturbances in the galactic structure, though a majority of the object appears undisturbed. Color gradients are evident; the central region exhibits a bluer hue in comparison to the more extended, outer regions, which display a shift towards redder tones. This suggests that the center of the galaxy hosts a population of younger, hotter stars. The inferred high star formation rate in the center is consistent with its bluer color. The redder outer areas imply a comparatively older stellar population. Overall, the galaxy shows characteristics consistent with an elliptical galaxy experiencing an episode of central star formation.
