The galaxy presents as a primarily smooth, centrally concentrated object. Its morphology is predominantly elliptical, displaying a high degree of radial symmetry with a round appearance. There is little evidence of distinct spiral arms or a prominent disk structure. The color gradient suggests an older stellar population, with the core appearing more yellow, indicative of evolved stars. Faint hints of blue are present in the outer regions, likely due to the presence of younger stars. The galaxy exhibits no obvious signs of ongoing merger activity or major disturbances, although there are subtle irregularities, suggesting a potential minor disturbance. The light profile appears well-behaved, smoothly decreasing in intensity from the center outwards with a half light radius of approximately 6.7 kpc. The galaxy is approximately 0.3 redshift, indicating that it's in the medium distance from our own galaxy.
