This galaxy exhibits a distinct, albeit somewhat diffuse, structure. It presents as a centrally concentrated system with a noticeable bulge, characterized by a yellowish-white hue, suggesting an older stellar population. Extending outwards from the central bulge is a fainter, less defined disk component. The disk exhibits a bluer coloration, potentially indicating the presence of younger, hotter stars and ongoing star formation regions. The overall morphology seems to indicate a spiral or lenticular galaxy type, although the image resolution limits definitive classification. There are hints of spiral arm structures, though they appear somewhat disrupted or flocculent rather than well-defined. No strong evidence of a major merger is visible; however, some minor asymmetry or disturbance in the outer regions is present, possibly suggestive of a past interaction or minor merger event. The galaxy does not appear to be a classic elliptical galaxy due to the presence of disk features.
