The galaxy presents a somewhat elliptical morphology, suggesting it may be an early-type spiral or lenticular galaxy. It displays a distinct central bulge region that appears yellowish in color, possibly indicative of an older stellar population dominating this area. The disk surrounding the bulge exhibits a bluer hue, which could point to the presence of younger, hotter stars and ongoing star formation. There are hints of subtle structural features within the disk, potentially indicating faint spiral arm segments or dust lanes, but these are not very pronounced. The galaxy appears relatively undisturbed, showing no clear signs of major mergers or tidal interactions.
