The galaxy presents as a lenticular or potentially an elliptical galaxy, exhibiting a smooth, elongated morphology with a high degree of central concentration. The dominant color appears yellowish-orange, suggesting an older stellar population and reduced ongoing star formation. The galaxy's axial ratio is relatively high, indicating a significant deviation from a spherical shape. There is little to no evidence of spiral arms or prominent dust lanes. No clear signs of tidal disturbances or ongoing major mergers are visible, although minor irregularities cannot be ruled out at this resolution. The galaxy's overall appearance is consistent with a passively evolving system.
