This galaxy presents a roughly elliptical morphology with a central, bright core. The core exhibits a high surface brightness, suggesting a dense concentration of stars and potentially an active galactic nucleus, though further spectral analysis is needed to confirm this. Surrounding the core is an extended halo or disk component. The overall color appears bluish-white, indicative of a population of relatively young, hot stars. Faint, irregular features are observed in the outer regions of the galaxy, possibly indicating minor gravitational disturbances or ongoing interactions with smaller satellite galaxies. These features are not strongly pronounced, suggesting that the galaxy is relatively undisturbed. The size appears modest relative to other galaxies, implying that it may be a dwarf galaxy. No prominent spiral arm structure is visible.
