The galaxy presents as a relatively bright, isolated object with a somewhat smooth morphology. Its color index suggests a redder population of stars, potentially indicating an older stellar population or significant dust obscuration. The galaxy appears elliptical in shape, although not perfectly spherical. There is a hint of a faint, diffuse halo surrounding the core, but no obvious signs of spiral arms or a prominent disk structure are visible. There may be a minor tidal interaction or disturbance occurring, as evidenced by a slight asymmetry in the outer regions, but further investigation would be needed to confirm this.
