The galaxy appears as an elliptical-like structure, exhibiting a predominantly smooth morphology without prominent spiral arms or a distinct disk. It shows a fairly circular shape with only a slight elongation. The light distribution suggests a concentrated central region gradually fading outwards. The color is biased towards the redder end of the spectrum, suggestive of an older stellar population and/or significant dust obscuration. No tidal tails or other obvious signs of recent major mergers are visible, though some minor disturbances cannot be ruled out based on the image alone.
