The galaxy appears to be a spiral galaxy viewed at a high inclination, potentially close to edge-on. A central bulge is discernible, exhibiting a yellowish hue indicative of an older stellar population. A disk surrounds the bulge. This disk shows hints of spiral arm structure, with bluer regions suggesting ongoing star formation, contrasting against the more diffused yellowish light. The galaxy does not appear to be undergoing any major merging events, although there may be minor irregularities in its structure. There does not appear to be strong disturbances in its disk. The overall morphology suggests a fairly well-defined structure, with some degree of disk prominence.
