The galaxy presents as a relatively smooth, elongated structure with a bright central bulge. The morphology leans toward an elliptical or lenticular type, with a high degree of central concentration. No distinct spiral arms or prominent dust lanes are discernible in the image. There's a subtle color gradient from the central region outward, suggesting a distribution of stellar populations and potential ongoing, but low-level, star formation. The overall light distribution is fairly uniform, lacking obvious signs of major tidal disturbances or active galactic nuclei. The axial ratio suggests a moderate inclination angle relative to our line of sight. Overall, this galaxy appears to be a mature system.
