The galaxy presents as a moderately sized, lenticular system with a redshift indicating significant distance. Its morphology appears largely smooth, with a notable lack of prominent spiral arms or distinct substructures. The overall shape is elongated, approximating a cigar-like form with axial asymmetry. The central region exhibits a concentrated, luminous bulge of a yellowish hue, suggesting an older stellar population. Moving outward from the core, the light profile gradually diminishes. There is a subtle color gradient from the center outwards, with bluer light appearing more prominent along the edges. No clear signs of active merging or major tidal disturbances are apparent, though some minor asymmetries in the outer regions may indicate a past interaction. The system's overall light profile indicates a relatively high mass and a low, but potentially non-negligible, rate of star formation.
