The galaxy presents as a somewhat diffuse, yet centrally concentrated object. The core exhibits a warmer, yellowish hue, suggesting an older stellar population or dust obscuration. Moving outward from the core, the galaxy transitions to a bluer color, with hints of green, potentially indicating more recent star formation activity. The morphology is not distinctly spiral or elliptical. The galaxy does appear somewhat disturbed, with non-uniform light distribution. There is no clear sign of any merger, but a minor disturbance might be present. The galaxy is neither distinctly smooth nor showing prominent spiral arms. The general shape is roughly circular, but its edges are fuzzy. Overall, this galaxy shows some signs of ongoing star formation and past disturbances.
