The galaxy presents as a singular, relatively smooth and round object with a concentrated central bulge. The color profile suggests an older stellar population, potentially dominated by redder stars. There is minimal evidence of spiral arms or significant disk structure. Faint, diffuse light extends outwards from the core, suggesting a halo of stars or tidally stripped material. There are no obvious signs of recent major merger activity. There is some evidence of slight structural disturbance. Overall, the galaxy appears to be a massive system, likely with minimal active star formation.
