This galaxy appears to be a relatively massive system, likely an elliptical galaxy given its smooth appearance and lack of distinct spiral arms. The light distribution suggests a centrally concentrated morphology. The galaxy exhibits a slight elongation. The core of the galaxy shows a yellowish-orange hue, potentially indicating an older stellar population, with diminished star formation. There is evidence of subtle disturbances or minor interactions, although the overall structure appears generally undisturbed. The galaxy appears to be a red galaxy, which has been shown to correlate with old galaxies dominated by evolved stars. 
