The galaxy presents as a single, relatively smooth, and centrally concentrated object. Its morphology appears largely spheroidal, with a high degree of roundness and no obvious disk component. There is no noticeable bar structure. The galaxy exhibits a color gradient, transitioning from a bluer core to redder outer regions. The overall luminosity suggests this is a massive galaxy, potentially an elliptical. The lack of strong irregularities or tidal features indicates it is not currently undergoing a major merger. There might be some minor signs of disturbance in its morphology. The central part of the galaxy appears bright, suggesting the presence of a concentration of stars. The outer regions are less defined and fade into the background sky.
