The galaxy presents a morphology that is neither purely elliptical nor a well-defined spiral. There is evidence of tidal distortions, suggesting an ongoing interaction or merger event. Two distinct nuclei or bright central regions are visible, appearing somewhat offset from each other. The overall color distribution shows a mix of blue and yellow hues, with the central regions appearing more yellow. The blue hues are suggestive of ongoing star formation in the outer regions, while the yellower centers are likely indicative of an older stellar population. There is no apparent dust lane. The galaxy appears to be in a stage of dynamic evolution.
