The galaxy appears as a relatively smooth, elliptical structure. Its core is a concentrated, luminous orange-yellow, suggesting an older stellar population dominates the central region. The galaxy exhibits a slight elongation, with a generally undisturbed morphology. There is evidence of some faint, bluer light in the outer regions, hinting at the presence of a younger stellar population or ongoing star formation, albeit at a low rate. No significant spiral arms or bar structures are discernible. There are no obvious signs of a major ongoing merger, though a subtle asymmetry might indicate a past minor interaction or disturbance. The overall appearance is consistent with an evolved galaxy, likely a massive system with a relatively low specific star formation rate.
