The galaxy appears to be a relatively smooth, elliptical-type galaxy with a bright, concentrated central bulge. The galaxy exhibits a radial color gradient, transitioning from a yellowish core region to a redder outer halo. There is a slight elongation visible in the galaxy's overall shape. The absence of distinct spiral arms or prominent dust lanes suggests a more evolved stellar population and a low rate of ongoing star formation. There is no apparent interaction with any other galaxies, and the overall morphology suggests it is an isolated system. There are no visible signs of major disturbances or merging events.
