The galaxy presents as a relatively smooth, centrally concentrated object. The light profile appears to be generally ellipsoidal. A prominent central bulge is visible, exhibiting a strong concentration of light and a yellowish-orange hue, suggesting an older stellar population.  There is a gradual decrease in surface brightness from the core outwards. The outer regions appear significantly fainter. No distinct spiral arm structures or prominent dust lanes are observed. Overall, it appears to be a relatively massive galaxy with a modest amount of star formation. No obvious signs of tidal interactions or recent merger events are seen.
