The galaxy presents as a single, prominent, elliptical-like structure in the image, with a relatively smooth, diffuse light distribution. There is indication of a possible merger event, with a slightly disturbed morphology visible in its structure. The galaxy is relatively round. The color gradient suggests a population of older stars, emitting light more towards the red end of the spectrum. The galaxy lacks distinct spiral arms or prominent dust lanes, indicative of an elliptical type galaxy. Overall, the galaxy appears to be a relatively massive and old stellar system, residing at a moderate redshift.
