The galaxy presents as a fairly smooth, centralized structure with a generally round morphology. The core exhibits a brighter, concentrated luminosity, suggesting a higher density of stars in the central region. A gradual decrease in light intensity extends outwards from the core, with no distinct spiral arms or bar features immediately apparent. The overall color profile indicates the presence of both older stellar populations, suggested by the redder hues, and some younger populations, indicated by bluer tinges especially in the outer regions. No major disturbances or tidal features are visible, suggesting it is likely not currently undergoing a major merger event, though minor irregularities may be present. The absence of prominent dust lanes contributes to the smooth appearance. 
