The galaxy presents as a somewhat elongated structure, suggestive of a disk galaxy viewed at a significant angle. The central region exhibits a concentrated bulge, appearing smoother in texture. Moving outwards, the galaxy shows hints of spiral arm structure, although these are not sharply defined, appearing rather diffuse. The color distribution shows a gradient. The central bulge appears more yellow/orange, indicative of an older stellar population. The outer disk appears slightly bluer, suggesting the presence of younger, hotter stars and ongoing star formation. Overall, the galaxy exhibits a moderate level of disturbance, possibly due to past minor merger events.
