The galaxy presents as a relatively smooth, centrally concentrated object. The light distribution appears to be quite regular, with a general elliptical morphology. There is little evidence of strong spiral arm features or prominent dust lanes. The galaxy is somewhat elongated but is mostly round. There are no obvious signs of major mergers or tidal disturbances within the galaxy's immediate vicinity, although there is some evidence of minor irregularities in its outer regions. The light is brightest in the center of the galaxy, with color gradients suggesting a stellar population variation with radius. Overall, it appears to be a well-defined galaxy with an undisturbed and seemingly stable morphology.
