This galaxy exhibits an elliptical morphology, with a smooth, diffuse light distribution that lacks well-defined spiral arm structures. The galaxy's core is relatively bright and concentrated. Based on its apparent morphology, it likely consists primarily of older stellar populations. There is some indication of a possible interaction or merger event. The object appears to have some disturbances in its overall shape, possibly with two primary concentrations. There is faint evidence of extended diffuse emission around the main body of the galaxy, suggesting a stellar halo or tidal features associated with the potential interaction. The galaxy appears reddish in color, indicative of an older stellar population, and a lack of active star formation. The object is at a considerable distance, as evident in the redshift data.
