The galaxy presents a generally elliptical morphology, appearing somewhat elongated. The central region exhibits a brighter, more concentrated luminosity, suggesting a significant stellar density or potentially an active galactic nucleus, though further spectral analysis would be required to confirm the latter. The light distribution falls off gradually toward the outer edges of the galaxy, with hints of disturbed features and asymmetry observed in the outer halo. There are signs of on-going or recent interaction with another galactic body, potentially merging. The color gradient across the galaxy shows an irregular distribution of light in the blue-green region, suggesting active star formation. This blue color is more dominant in some regions of the galaxy than others.
