The galaxy presents as a largely smooth, elliptical morphology. The light is concentrated toward the center, forming a bright nucleus that appears somewhat spherical. The color profile indicates that the galaxy is likely composed predominantly of older stellar populations, emitting light primarily in the redder wavelengths, with minimal blue light indicative of younger, hotter stars. There is little evidence of significant dust lanes or spiral arm structures, suggesting a relatively quiescent star formation history. A slight deviation from perfect circularity is observed, and the general texture shows few if any strong disturbances or tidal features. This morphology is consistent with a high likelihood that this is a mature galaxy with a relatively high stellar mass and a low ongoing star formation rate.
