This galaxy appears to be a spiral galaxy viewed at a moderate inclination. The central bulge is prominent and exhibits a yellowish-orange hue, suggesting an older stellar population. The disk is visible, though somewhat fainter, extending outwards from the bulge. There is a suggestion of spiral arm structure, but the resolution is insufficient to clearly resolve distinct arms. The galaxy appears relatively smooth in overall appearance, though there is some patchiness in the disk, possibly indicating regions of ongoing star formation. The color of the galaxy is generally redder than expected for an actively star-forming spiral galaxy, which could be the result of reddening due to dust, an older stellar population, or a combination of factors. There is no obvious evidence of a major ongoing merger or tidal disturbance, although the possibility of a minor interaction cannot be ruled out given the subtle asymmetries in the disk.
