The galaxy presents as a relatively smooth, elliptical object. Its light distribution appears centrally concentrated, with a gradual falloff in intensity towards the outer regions. The core exhibits a bright, intense luminosity, hinting at a possible active galactic nucleus or a dense stellar population. There is a slight flattening of the galaxy along its major axis; its overall shape leans towards an elongated spheroid. While no distinct spiral arms or prominent dust lanes are visible, there may be some subtle color variations within the galaxy, suggesting differing stellar populations or compositions in certain regions. The outer edges display a diffused and fuzzy appearance, indicative of a less densely populated halo. Overall, the galaxy appears to be a relatively evolved system.
