The galaxy presents a generally smooth morphology. It exhibits a slightly elongated, but overall rounded shape. A distinct central concentration of light is observed, suggesting a possible bulge component. There are no prominent spiral arms or distinct features indicative of a disk-dominated system. The galaxy's color appears somewhat reddish, implying an older stellar population and potentially ongoing, but relatively low, star formation activity. The absence of strong tidal features suggests it is not currently undergoing a major merger, though minor disturbances are difficult to rule out at this resolution. The luminosity indicates a relatively massive galaxy.
