The galaxy exhibits a centrally concentrated morphology, appearing largely smooth with a gradual decrease in luminosity from the core outwards. The core region presents a yellowish hue, potentially indicating an older stellar population. Surrounding the core, a less defined, bluer region suggests the presence of younger stars and possibly ongoing star formation. The galaxy does not appear to have a pronounced disk-like structure or spiral arms. There may be very slight irregularities in the outer regions. No obvious signs of a recent or ongoing major merger event are visible, but subtle asymmetries might indicate minor gravitational disturbances. Overall the galaxy presents as a large, relatively evolved system.
