The galaxy presents as a moderately luminous, elliptical system exhibiting a smooth, generally featureless morphology. The central region displays a concentrated, bright core, indicative of a likely significant stellar population density. The isophotes appear elongated, suggesting a prolate spheroid shape rather than a perfectly circular form. The color profile transitions from a yellowish-orange in the core to a slightly redder hue in the outer regions. There is no discernible evidence of spiral arm structures, dust lanes, or active star formation regions in the available imagery. Overall, this system appears consistent with a relatively quiescent, early-type galaxy at intermediate redshift.
