The galaxy appears as a single, slightly elongated, diffuse object with a primarily smooth morphology. The light distribution is concentrated centrally, presenting a bright, almost circular core. There appears to be evidence of a secondary, smaller core suggesting a potential merger event or interaction with a companion galaxy. The overall color is yellowish-orange, indicative of a galaxy dominated by older stellar populations. Hints of possible tidal tails or minor disturbances are observed, suggesting this galaxy is not entirely quiescent and that there may be ongoing or recent gravitational interactions occurring.
