The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, relatively featureless structure. The light distribution suggests a concentration towards the center, with a bright core indicative of an older stellar population. The overall shape deviates slightly from a perfect circle, appearing somewhat elongated, perhaps cigar-shaped, suggesting a degree of intrinsic flattening or a potential minor interaction. There's no clear evidence of spiral arms or significant dust lanes. The galaxy is observed at a moderate redshift, indicating a substantial distance and lookback time. The estimated size is consistent with that of a large galaxy. Star formation appears to be subdued. The absence of prominent morphological disturbances suggests it is not currently undergoing a major merger.
