The galaxy appears as a somewhat elongated, lenticular or possibly edge-on spiral structure. A bright central bulge dominates the overall light profile, suggesting a significant population of older stars concentrated towards the center. The disk component is visible, though not sharply defined, with hints of dust lanes or spiral arms. The disk exhibits a smoother texture compared to the bulge, indicating a more dispersed stellar population. The colors are consistent with a mix of stellar ages, with the central bulge showing a yellow-orange hue and the disk exhibiting bluer tones. There may be slight disturbance to the shape suggesting it underwent some sort of disturbance in the past, but is otherwise pretty smooth. Overall, it does not look like it is merging with another object.
