The galaxy presents as a flattened, elongated structure, highly inclined relative to the line of sight. It exhibits a noticeable central bulge, which appears to be a concentrated region of higher luminosity and density. The overall color gradient suggests a concentration of older stellar populations within the bulge, indicated by its yellowish-orange hue. The surrounding disk component appears fainter and bluer, potentially indicative of ongoing or recent star formation. The disk is relatively smooth and lacks distinct spiral arm structures discernible in the image, suggesting it may be a lenticular type galaxy. The galaxy displays a defined edge, implying the absence of a significant extended halo. There is little evidence of significant dust lanes or obscuration within the galaxy, based on the relative transparency of the disk. The galaxy does not appear to be actively undergoing a major merging event, though some minor disturbance within the disk cannot be ruled out.
