The galaxy presents as a slightly inclined, lenticular-like structure. It exhibits a bright, concentrated central bulge that gradually diffuses outwards, forming a somewhat elongated disk. A noticeable color gradient is observed, with the central region appearing whiter, suggesting an older stellar population. Progressing outward, the disk appears more blueish, hinting at the presence of younger, hotter stars and potential star-forming regions. The disk seems relatively smooth with no distinct spiral arm structures, consistent with a partially disrupted spiral or an elliptical galaxy. There is a small area of reddish hue near the main galaxy body on one side, which may be indicative of dust lanes or an area of significant star formation. The overall morphology suggests that the galaxy may be undergoing some form of interaction or disturbance, although the general form is fairly regular.
