This galaxy exhibits a generally smooth morphology, with a somewhat elliptical shape. There is a clear central bulge that appears more concentrated and has a distinct reddish-orange hue, suggesting an older stellar population is concentrated at the center. A less defined disk is visible, displaying hints of bluer colors indicating the presence of younger stars and likely ongoing star formation within the outer regions. The galaxy appears relatively undisturbed, showing no strong signs of major mergers or tidal interactions. However, there may be subtle signs of minor disturbances present in the galaxy. The galaxy's color gradient transitions from the reddish core to a slightly bluer periphery. Overall, the galaxy presents as a relatively massive system with evidence for both an older bulge and a more actively star-forming disk component.
