The galaxy appears as a centrally concentrated object with a generally smooth morphology, although faint features or a disk-like structure may be present upon closer inspection. The central region exhibits a relatively high surface brightness, showing a pinkish hue, which may indicate the presence of an older stellar population or a centrally located active galactic nucleus. The overall color of the galaxy seems to be moderately blueish, suggesting some ongoing star formation activity. The general form of the galaxy seems to be in between round and elongated. There is no clear visual evidence of major mergers or significant tidal disturbances, though subtle asymmetries or minor perturbations may be present in the outer regions.
