The galaxy presents as a relatively smooth, centrally concentrated object. It appears as an elliptical-like galaxy with a diffuse, extended halo. The color profile suggests a population of older stars, indicated by the redder hue and the presence of some young stars, which is indicated by the bluer hue in the very center of the galaxy. There is no prominent dust lane or spiral arm structure visible. There does not appear to be any evidence of a major ongoing merger or strong tidal disturbance from the image, the galaxy exhibits a generally undisturbed morphology with only a minor interaction potentially occurring. The shape of the galaxy is generally elliptical, trending toward round, without significant elongation. The object has a calculated redshift of approximately 0.17, indicating a substantial distance. This object is a luminous galaxy.