The galaxy presents an elliptical morphology, appearing generally smooth in texture, with little evidence of spiral arms or distinct features. The central bulge exhibits a bright, concentrated luminosity, appearing approximately round with some elongation. The light profile gradually decreases outward from the bulge, blending into a fainter halo region. There are faint hints of a disk, but it is relatively featureless. There is no visible dust or active star-forming regions, suggesting a low ongoing star formation rate. The overall color suggests an older stellar population. There are hints of minor gravitational disturbance.
