The galaxy presents a largely smooth morphology, with a dominant central bulge exhibiting a high degree of symmetry. It appears elliptical, with a somewhat diffuse edge. The light is concentrated towards the center, indicating a potentially old stellar population, although a slightly bluer hue is noted. There is no sign of spiral arms, bars, or any ongoing major merging activity. A subtle distortion or minor disturbance is not ruled out. It shows a moderate level of star formation.
