The galaxy presents as a relatively well-defined elliptical structure, with a smooth, diffuse light distribution indicative of an older stellar population. There is a slight elongation, but overall the galaxy appears largely spheroidal. A central concentration of light suggests the presence of a galactic nucleus. While it is difficult to discern detailed features, the lack of prominent spiral arms or dust lanes reinforces its classification as an elliptical galaxy. Based on its color, it presents a spectral makeup that suggests ongoing, moderate levels of star formation with a corresponding mass as well. The galaxy appears to be in the later stages of a merger or collision, which has disrupted any disk structure that may have existed prior to the interaction.
