The galaxy presents as a relatively smooth, elongated structure. The color profile indicates a mix of stellar populations, with a central concentration of what appears to be older, redder stars. There's a noticeable blueish tinge to the outer edges of the galaxy, suggesting the presence of younger, hotter stars and possibly ongoing star formation in the disk. The lack of distinct spiral arms or a prominent bulge suggests it may be an elliptical galaxy or a lenticular galaxy viewed edge-on. There appear to be no major disturbances or signs of recent merger activity. The overall morphology indicates a galaxy that is relatively evolved.
