The galaxy presents a roughly elliptical morphology, with a bright, concentrated central bulge. The bulge exhibits a distinct reddish hue, possibly indicating an older stellar population dominated by red giant stars and/or significant dust obscuration. Surrounding the bulge is a fainter, extended disk-like structure. This disk appears to be oriented approximately edge-on. The disk component displays a greenish tint, which may suggest ongoing star formation activity within the disk. Evidence of dust lanes or other fine details within the disk is limited due to the image resolution, but subtle variations in color and brightness are visible. There is a minor asymmetry observed, perhaps indicating gravitational interactions.
