The galaxy presents as a centrally concentrated object, exhibiting a smooth morphology. Its overall shape approximates an ellipse, appearing more elongated than perfectly circular. The light distribution suggests a relatively uniform stellar population, without prominent spiral arms or distinct features such as dust lanes. The color gradient indicates a possible population of older stars with only low levels of star formation occurring, as evidenced by the redder hue in the outskirts, and the relatively low brightness of the galaxy. There does not appear to be evidence of any major mergers. Some minor disturbances are not completely ruled out based on the shape of the galaxy, but no prominent interactions with other galaxies are observed in this image.
