The galaxy appears as a centrally concentrated object. It exhibits a generally smooth morphology, with a lack of distinct spiral arms or a prominent disk structure. The overall shape appears somewhat rounded, though not perfectly circular. There is a hint of elongation or a slight deviation from perfect roundness. The color profile suggests that the galaxy is dominated by older stellar populations, likely residing within a spheroid-like structure. There is little evidence of ongoing, significant star formation, with redder colors predominating. No obvious signs of major mergers or significant tidal disturbances are observed in this image. However, subtle asymmetries or minor disturbances cannot be ruled out at the given resolution. The estimated size is a few kiloparsecs in radius.
