The galaxy presents a generally smooth, elliptical morphology with a centrally concentrated luminosity profile. The light distribution is primarily homogeneous, lacking prominent spiral arm structures or distinct dust lanes. A gradual decrease in surface brightness is observable from the core outwards. The color gradients are subtle, but there appears to be a slightly bluer tint in the outer regions of the galaxy compared to the more yellow-white core. The galaxy appears largely undisturbed, with no obvious signs of major mergers or tidal interactions. There is a slight indication of some minor distortion, but overall the galaxy maintains a regular, relaxed structure. The galaxy shows some star formation, but appears to be a relatively inactive galaxy.
