The galaxy presents as a moderately bright, disk-shaped object. The central region exhibits a concentrated, bright yellowish core, suggesting an older stellar population and potentially a supermassive black hole actively accreting material. The disk surrounding the core appears smooth, and is not clearly resolved into spiral arms or distinct star-forming regions. There is some subtle color variation within the disk, with hints of bluer light on one side and redder light on the opposite side, possibly indicating some differential star formation or dust obscuration. The overall morphology suggests the galaxy is likely an intermediate-type spiral or possibly a lenticular galaxy, with a smooth light profile and lacking prominent spiral structures. There may be some tidal disturbances or minor interactions with smaller galaxies.
