This galaxy presents as a single, relatively smooth object with a concentrated central region. There is evidence of a possible ongoing merger or tidal interaction, with asymmetric light distribution around the primary galactic body, suggesting a non-equilibrium dynamical state. The color profile suggests a relatively evolved stellar population. Its morphology appears to be predominantly spheroidal, with a lack of discernible spiral arm structure. The overall appearance suggests a system with relatively low specific star formation rate.
