The galaxy presents as a smooth, elliptical-like structure with a high degree of central concentration. The color profile indicates a dominant population of older stars, evidenced by the redder hue. The object's morphology suggests that it is an early-type galaxy, either elliptical or lenticular. There is no clear evidence of spiral arms or prominent dust lanes, and the lack of discernible features suggests a relatively quiescent star formation history. The galaxy exhibits a moderate degree of elongation and a notable lack of irregularities in its overall shape. The object has a definite structure which leads one to believe it is a galaxy as opposed to an artifact. 
