This galaxy presents as a somewhat elongated, disk-like structure, viewed at a significant angle. It displays a relatively smooth overall appearance. There appears to be a central bulge region that exhibits a more concentrated, reddish hue, suggesting an older stellar population. Extending outward from this central region, a flattened disk structure is evident. This disk shows a gradient of color, transitioning from the reddish tones in the center to a greenish and bluish hue at the edges. This suggests the presence of a younger, hotter stellar population and potentially ongoing star formation in the outer regions of the disk. There is little evidence of distinct spiral arm structure or significant dust lanes. Overall, this galaxy could be described as an early-type spiral or a lenticular galaxy that is actively forming stars. There is some slight evidence of possible minor gravitational interaction with a nearby object, although further investigation would be needed to confirm this.
