The galaxy appears to be a luminous object at a considerable distance, exhibiting a redshift of approximately 0.188. Morphologically, the galaxy presents a predominantly smooth appearance, suggesting it may be an elliptical galaxy or a spiral galaxy viewed face-on with a dominant bulge. However, there are subtle indications of features or a possible disk-like structure present within the galaxy's overall form. It is neither perfectly round nor highly elongated. There appears to be a slight disturbance present within the galaxy, suggesting that the system may be in the early stages of an interaction. The galaxy's color profile indicates a redder hue, implying a population of older stars and a relatively low rate of star formation.
