The galaxy presents a generally smooth morphology, appearing largely elliptical in shape. There is a noticeable concentration of light towards the center, suggesting a prominent galactic nucleus. The color profile indicates a mix of stellar populations, with the central regions displaying a yellowish or golden hue, potentially indicative of older stars. The outer regions exhibit a bluer tint, hinting at the presence of younger, hotter stars and ongoing, or recent star formation. A slight asymmetry is observed, potentially suggesting some minor tidal interaction or past merger event but generally seems stable in appearance. 
