The galaxy appears to be an elliptical type, characterized by its smooth, somewhat round morphology and a lack of prominent spiral arms or a distinct disk structure. It exhibits a centrally concentrated luminosity profile, suggesting a high degree of stellar density within the galactic core. The galaxy shows a relatively uniform color distribution, with a subtle bluer tint around the edges, hinting at ongoing, albeit subdued, star formation activity at its periphery. The overall structure is mostly undisturbed, though with hints of minor interactions.
