The galaxy appears to be an elliptical galaxy, characterized by a smooth, centrally concentrated light distribution. It exhibits a generally round morphology, though not perfectly spherical. There are no obvious spiral arms or a distinct disk structure visible. The galaxy's core region displays a brighter, more concentrated luminosity, fading gradually towards the outer edges. The dominant color is a yellow-orange hue, indicative of an older stellar population, with lower levels of recent star formation. There is no indication of active galactic nuclei or substantial dust lanes. No major mergers or tidal disturbances can be observed, with the overall structure appearing relatively undisturbed. The galaxy exhibits a level of apparent faintness, suggesting it is relatively distant.
