The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated, bright central bulge, surrounded by a fainter, more diffuse halo. The color profile suggests a population of older stars, with a redder hue dominant in the central region, grading slightly towards a bluer color in the outer halo. No prominent spiral arms or dust lanes are discernible in the image. There is an indication of a faint, extended structure surrounding the main body of the galaxy, although the signal is weak. The overall impression is that of a relatively evolved galaxy, potentially a lenticular or elliptical type, with a well-established stellar population and minimal ongoing star formation. A general round shape is observed for this system.
