This galaxy appears to be a relatively luminous elliptical galaxy at a redshift of approximately 0.27. The main body of the galaxy exhibits a smooth, centrally concentrated light profile, indicative of an older stellar population. There are no prominent spiral arms or a defined disk component. The galaxy presents with a largely spheroidal shape. There are indications of minor disturbances in the galaxy's morphology, possibly due to a past or ongoing minor merger event. Faint, diffuse light extends outward from the central region, suggesting a galactic halo. The central core appears yellowish-red, while the outer regions show a slight hint of blue, potentially indicating some residual star formation activity, albeit at a low rate.