The galaxy presents as a smooth, elliptical morphology, with a concentrated central bulge that gradually diffuses into the outer regions. The core exhibits a yellowish hue, suggesting an older stellar population. A slight elongation is observed, indicating it is not perfectly spherical. There is no visible evidence of spiral arms or a disk-like structure. The overall appearance indicates minimal ongoing star formation, consistent with a relatively quiescent galaxy. There is no apparent interaction or merging event currently occurring with other galaxies or celestial bodies.
