This galaxy exhibits characteristics of a merging system or a galaxy undergoing significant disturbance. The central region displays a high degree of sphericity, with a smooth distribution of light. However, distinct features suggest more complex interactions. A possible tidal tail or bridge extends outwards, and the overall morphology indicates a recent or ongoing merger event with another galactic body. The galaxy's color is predominantly yellow-red, suggesting an older stellar population. The light distribution further implies that the central bulge has a well-established and gravitationally bound configuration. There are no clear spiral arm structures visible. Based on its features, it shows characteristics of a galaxy with a relatively quiescent star-formation rate, with the mass contained within a relatively concentrated central bulge.
