This galaxy appears to be a relatively compact and luminous object. The light is concentrated towards the center, with a smooth, diffuse halo extending outwards. The galaxy exhibits an overall elliptical shape, showing a structure between round and elongated. There is little evidence of spiral arm structures or strong dust lanes. The color profile is fairly uniform, with a slightly redder hue, particularly in the central region, suggesting an older stellar population. No obvious signs of recent or ongoing major merger activity can be observed, although subtle disturbances cannot be ruled out. 
