The galaxy appears to be a relatively smooth, elliptical type. It exhibits a high degree of radial symmetry, appearing largely circular in projection. There is a concentrated central bulge, with a gradual decrease in luminosity moving outward from the core. The color of the galaxy is predominantly yellow-red, suggesting an older stellar population. Subtle irregularities in the outer regions indicate the possibility of minor disturbances or interactions, but there are no distinct tidal tails or other signs of ongoing major mergers visible in this image. The overall structure suggests that the galaxy is likely well relaxed.
