The galaxy presents as a single, relatively symmetrical, elliptical-like object with a smooth light distribution and no apparent spiral arm structure or prominent dust lanes. The light is concentrated towards the center, suggesting a substantial bulge component. The galaxy exhibits a yellowish-white hue, indicative of an older stellar population, and low levels of current star formation activity. The object is likely a galaxy at an intermediate cosmological distance, with a noticeable redshift. The morphology of the galaxy is smooth, featureless and round. There is no evidence of a recent major merger or interaction with another galaxy based on the undisturbed structure.
