The galaxy presents as a smooth, concentrated distribution of light with a slight elongation in its morphology. The color profile suggests a primarily older stellar population, with a notable lack of intense blue regions indicative of recent, widespread star formation. There appears to be some indication of minor disturbances or perhaps the initial stages of a minor merger event, but without high resolution data it is difficult to classify. The galaxy is mostly circular with some cigar shaped qualities. The galaxy's overall appearance is consistent with an elliptical morphology.
