The galaxy presents a predominantly smooth, elliptical morphology with a centrally concentrated bulge. The color profile transitions from a yellowish hue in the core to a bluer periphery, suggesting the presence of younger stellar populations in the outer regions and potentially ongoing star formation. There is no obvious disk structure, and the absence of prominent spiral arms or bar features is evident. The galaxy exhibits a slight asymmetry in its overall shape, possibly indicating a minor gravitational interaction or recent accretion event. No major disturbances or signs of a major merger are apparent, though minor disturbances cannot be excluded. The galaxy is moderately luminous with a significant stellar mass, placing it within the range of typical elliptical galaxies at its redshift.
