The galaxy presents as a relatively compact object with a smooth, featureless morphology. There is no clear evidence of spiral arms or a well-defined disk structure. The galaxy exhibits a centrally concentrated luminosity profile, appearing brightest in the core region, with intensity gradually diminishing outward. The overall color appears slightly redder, possibly indicating an older stellar population with ongoing, but limited, star formation. There is a subtle hint of irregularity in the outer isophotes, potentially suggestive of minor tidal disturbances or past interactions. The round morphology dominates the image, with a slight deviation. The size appears to be within normal parameters for a galaxy at this distance. 
