The galaxy appears to be an interacting system, likely composed of two distinct galaxies in the process of merging. The primary galaxy exhibits a smooth, elliptical morphology with a concentrated central bulge. The color suggests an older stellar population, with a dominant yellowish hue, potentially indicative of low star formation activity. A secondary, smaller galaxy is visible, displaying a similar smooth morphology but with a slightly bluer color, hinting at the presence of younger stars or ongoing star formation. There's a subtle bridge of faint light that might be tidal debris connecting these two galaxies. The overall shape of the system is elongated, which could be a result of the gravitational interaction. There is no evidence of a strong spiral structure or prominent dust lanes in either component.
