The galaxy presents as a centrally concentrated object with a generally smooth morphology. The color profile indicates an older stellar population, with a strong contribution from redder wavelengths in the core. The outer regions display a slight bluer tint, suggesting the presence of a small population of younger, hotter stars; however, star formation appears to be relatively quiescent. The galaxy exhibits a near-circular shape without any obvious spiral arm structures or significant distortions, suggesting that it is likely an elliptical or lenticular galaxy. There is no obvious indication of an ongoing merger event or significant tidal disturbance, although there may be minor irregularities in the outer regions that could warrant further investigation. The galaxy exhibits a moderate size for its redshift.
