The galaxy presents a somewhat rounded morphology. It exhibits a primarily smooth texture in its overall appearance, with a slight suggestion of a central concentration. There is a subtle indication of internal structure, though it does not appear to be dominated by spiral arms or a prominent disk.  The galaxy's color profile displays a range from blue-ish, potentially indicating regions of recent or ongoing star formation, to more reddish hues, possibly associated with older stellar populations or dust obscuration.  There is no strong evidence of a major ongoing merger, although some mild asymmetries or disturbances could be present.
