The galaxy presents as an elongated, disk-like structure, likely a spiral or lenticular type viewed at a significant inclination. A central bulge is evident, exhibiting a concentrated luminosity. The color gradient suggests a younger stellar population in the central region, potentially indicating recent or ongoing star formation. Dust lanes appear subtly along the galactic plane, obscuring light from the stars behind them. The outer regions of the disk are less defined, with a gradual decrease in luminosity, suggesting older stellar populations and a lower density of star formation. The overall morphology leans towards a relatively smooth texture, with no apparent major disturbances or signs of an ongoing merger event.
