The galaxy presents as a diffuse, ellipsoidal structure with a relatively smooth, indistinct morphology. A noticeable central bulge is observed with a gradual fading towards the outer edges. There is a slight elongation to the galaxy's shape, appearing somewhat flattened. The color distribution indicates a concentration of older stellar populations towards the central region, exhibiting a yellowish-red hue. The outer regions appear slightly bluer, possibly indicating the presence of younger stars or ongoing star formation, though no distinct spiral arms or features are discernible within the limits of the image resolution. Overall, the galaxy appears to be an evolved system with a relatively high degree of central concentration and limited star formation activity. There might be a possibility of an ongoing or past merging event due to the galaxy's somewhat irregular shape.
