The galaxy presents as a single object, likely elliptical in overall shape. The core region exhibits a high degree of concentration with a bright, yellowish hue, suggesting an older stellar population. A fainter, bluer extension appears at one end of the galaxy, possibly an area of recent star formation or tidal debris resulting from a past merger event. The main body of the galaxy appears relatively smooth in texture, with no obvious spiral arm structures visible. The slight elongation and asymmetry suggest a potential interaction with another galaxy, or a recent disturbance in its morphology. Given the red shift, the observed colour suggests that the light emitted by the galaxy is redder, this could be due to its distance.
