The galaxy appears to be a relatively smooth, centrally concentrated system. Its light profile suggests a bulge-dominated morphology. The elliptical shape is nearly round. There is no prominent disk structure visible, nor any obvious spiral arms. There may be a hint of a subtle, outer halo, but it is very faint. No signs of tidal features or recent mergers are apparent. The color of the galaxy shifts subtly from bluer in the outer regions to redder towards the core, which may be indicative of an older stellar population in the center.
