The galaxy presents as a centrally concentrated object, appearing elliptical in shape though with some ambiguity due to the image resolution. The core region exhibits a bright, yellowish-white hue, potentially indicative of an older stellar population. The outer regions of the galaxy display a faint, diffuse blue halo. This may indicate areas of more recent, though not vigorous, star formation activity. The overall light distribution appears relatively smooth with no obvious signs of spiral arms or distinct dust lanes. There is a slight asymmetry to the overall structure, suggesting the possibility of a minor gravitational interaction.
