The galaxy presents as a relatively compact, luminous object with a generally elliptical morphology, appearing highly smoothed and exhibiting a high degree of central concentration, suggesting a spheroid-dominated system. Color gradients from the core to the outer regions of the galaxy are subtle, with the core appearing slightly more yellow in hue. There are no prominent spiral arm structures or significant dust lane features visible at this resolution. The galaxy appears to be relatively undisturbed, though subtle asymmetries in the light distribution could indicate minor gravitational interactions. The galaxy is reasonably red, suggesting an older stellar population.
