The galaxy presents as a relatively smooth, elongated structure, suggesting it could be an elliptical galaxy or a lenticular galaxy viewed edge-on. There is a noticeable color gradient, with a reddish core transitioning to a bluer hue in the outer regions. This may indicate a difference in stellar populations, with older, redder stars concentrated in the central bulge and younger, bluer stars populating the disk. The galaxy exhibits only minor disturbances, suggesting it has not undergone any recent major mergers. The luminosity profile appears relatively concentrated. The galaxy appears moderately massive with an intermediate rate of star formation. 
