The galaxy presents as a centrally concentrated, smooth object with a slightly elliptical morphology, though tending toward round. The core region exhibits a pronounced yellow hue, suggesting an older stellar population dominating this area. The light gradually fades from the center outwards, and the outer regions appear redder and less defined. No distinct spiral arms or bar structures are discernible, and there is no significant indication of ongoing major merger activity or tidal disturbances in the surrounding region. There appears to be a low amount of recent star formation occurring in the outer edges of the galaxy.
