The galaxy presents as an elliptical morphology, exhibiting a centrally concentrated luminosity profile. It has a smooth appearance with no apparent spiral arm structure or distinct dust lanes. The color gradient suggests an older stellar population dominating, as evidenced by the reddish hues in the central region. The galaxy's overall shape is somewhat elongated but leans towards a more rounded form. There may be slight disturbances in the outer halo, which could potentially indicate past minor mergers or tidal interactions. Star formation is very weak to nonexistent.
