The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that is significantly brighter than the surrounding halo. The galaxy's overall shape is generally round, with a slight deviation towards an intermediate elliptical form. There is no clear evidence of spiral arms or a prominent disk structure. The color profile suggests a population of older stars, with a lack of blueish areas typical for star-forming regions. There are no visible signs of any major disturbances or mergers that affect its shape. The galaxy exhibits no distinct morphological features. 
