The galaxy presents as a largely featureless, elliptical-like structure. It exhibits a concentrated central bulge that transitions smoothly to the outer regions. The dominant color is a yellow-white hue, indicative of an older stellar population with little active star formation in the central regions. Fainter blue light surrounds the yellow core of the galaxy. This blue color could indicate the presence of younger stars and ongoing star formation in these outer regions. No prominent spiral arms or dust lanes are discernible. The overall morphology is smooth and regular, suggesting a dynamically relaxed system. There is no indication of major tidal disturbances, mergers, or interactions with neighboring galaxies. The galaxy appears relatively isolated in this field.
