The galaxy presents as a centrally concentrated, luminous object. It appears largely smooth in morphology, with a primarily elliptical shape. There is a notable absence of distinct spiral arms or other prominent features typically associated with disk galaxies. The light distribution suggests a relatively uniform stellar population, possibly indicative of an older, passively evolving system with a low rate of star formation. The color profile appears slightly redder towards the galactic center, which might point to a higher concentration of older stars and dust in that region. There are slight hints of disturbance in the outer edges, but the overall form is mostly undisturbed. It shows no signs of active merging and is quite symmetrical. 
