This galaxy exhibits a roughly elliptical morphology, presenting a smooth, yet subtly textured appearance. The central region displays a bright, concentrated luminosity, indicative of a significant stellar population. Progressing outwards, the luminosity gradually diminishes, suggesting a radial decline in stellar density. Faint, diffuse structures with a blueish hue are distributed across the surrounding regions, potentially indicating the presence of younger stellar populations and ongoing star formation, though the smooth morphology would otherwise imply an older population. There does not appear to be any interaction with other objects or obvious signs of active galactic nuclei. There are no strong dust lanes or well-defined spiral arms. This suggests it might be a galaxy in transition, perhaps evolving from a spiral to an elliptical morphology or in the process of growing its bulge.
