The galaxy appears as a centrally concentrated object, exhibiting a smooth morphology. It presents an overall elliptical shape, with an estimated diameter of approximately 7 kpc. The light profile suggests an older stellar population, with a dominant yellow/red hue indicative of evolved stars. The galaxy is likely undergoing or has recently undergone a significant merger event, as evidenced by the irregular shape, with a secondary concentration offset from the primary nucleus. This disturbance indicates gravitational interaction influencing its current structure, which presents features potentially resulting from tidal forces. There is no significant evidence of ongoing star formation within the central region of the galaxy, as evidenced by the absence of bluer regions.
