The galaxy presents as an elliptical form, with a generally smooth appearance. The central region is more luminous, suggesting a concentration of stellar populations. The light distribution appears to be consistent with an older stellar population, with a redder hue overall. There is a possible indication of minor tidal interactions or disturbances in the outer regions, with faint, diffuse extensions or irregularities visible, most obviously on the far right. The galaxy does not appear to exhibit any prominent spiral arms or significant dust lanes. Overall, the morphology suggests a galaxy undergoing or having undergone a merging event. 
