This galaxy appears to be an elliptical or lenticular galaxy at a redshift of approximately 0.12. Its overall form presents a largely smooth and diffuse light distribution. There is no clear evidence of spiral arms or a prominent disk structure. The galaxy is more or less centrally concentrated, with the highest luminosity observed towards the core region. There's a slight elongation but, overall, it has an essentially rounded appearance. The outer regions fade gradually into the background sky, suggesting a rather smooth transition in stellar density. There appears to be a very weak hint of some disturbance, but this could be background noise or a very minor interaction. Based on this image, the galaxy exhibits light consistent with an older stellar population.
