The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a yellow-orange hue, suggesting an older stellar population with minimal ongoing star formation. The overall shape is generally round, though not perfectly spherical. There is some subtle asymmetry apparent in the outer regions, which could be indicative of a minor interaction or tidal disturbance, but it isn't a strong disturbance. The galaxy is not a late-stage merger.
