The galaxy appears to be a relatively smooth, centrally concentrated system. Its shape is elongated, with a noticeable deviation from perfect circularity, tending towards a cigar-like morphology. The central region exhibits a higher surface brightness, indicating a dense stellar population or active galactic nucleus. There are hints of a disk-like structure, though the smoothness suggests the spiral arms, if present, are tightly wound or diffuse. No major disturbances or signs of ongoing merger activity are readily apparent, though minor interactions cannot be ruled out. The overall color is suggestive of a galaxy dominated by an older stellar population, but there is also evidence of ongoing star formation activity within.
