The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and rounded morphology. The galaxy's light is concentrated in the center with a decreasing luminosity gradient towards the edges. The central region is yellowish-orange, possibly indicating an older stellar population. Faint, diffuse arms may be visible along the edges of the central region. The galaxy has an estimated redshift of 0.23, placing it at a significant cosmological distance. The isophotes appear generally elliptical. There is no evidence of a prominent disk component, active star formation, or major merger activity. The morphology is suggestive of a relatively evolved galaxy with a high mass.
