The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated structure. There is a strong central bulge that appears roughly spherical, gradually fading into an extended, diffuse halo. The color profile suggests a population of older stars, evidenced by the yellow-red hue, particularly concentrated within the central bulge. There is some blue light, especially in the outer disk, indicating recent star formation. No distinct spiral arms are visible; however, there is a slight suggestion of a disk structure. There is no obvious morphological distortion indicative of a recent major merger, although there are minor irregularities present. The galaxy's overall appearance suggests a system in a relatively quiescent state, with a moderate rate of star formation.
