The galaxy presents a predominantly smooth morphology, appearing as a single, concentrated object. It exhibits a roughly round shape, showing a slight deviation from perfect circularity. A discernible core of concentrated light is visible, surrounded by a more diffuse halo. The color profile is dominated by warmer tones, particularly in the central region, suggesting an older stellar population. Fainter, slightly bluer light surrounds the central bulge, potentially indicating a small amount of ongoing star formation in the outer regions. There is no strong evidence of spiral arms or a pronounced disk structure. No significant tidal disturbances or merger activity are immediately apparent in the immediate vicinity of the galaxy.
