The galaxy presents a moderately inclined disk-like structure. The central region exhibits a brighter, somewhat diffuse concentration of light, likely indicating a bulge component. The overall color suggests a predominantly older stellar population, with hints of bluer regions in the disk, potentially indicating areas of recent star formation. The galaxy appears to be relatively undisturbed, showing no major signs of tidal interactions or mergers, although subtle asymmetries within the disk cannot be ruled out at this resolution. The shape tends towards round, though not perfectly circular, with elongation. The galaxy's structure seems to be dominated by smoothness, with less clear definition of spiral arms.
