The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, diffuse light distribution with a high degree of central concentration. The overall shape is somewhat elongated, appearing more "in-between" than perfectly round, with a slight cigar-like tendency. There is no distinct disk or spiral arm structure visible, and the galaxy appears to be dominated by an older stellar population, indicated by the yellowish-orange hue towards the central region. The outer regions are fainter and bluer, possibly due to the presence of younger stars. There are no indications of major disturbances or merging activity, though there might be minor structural irregularities, suggesting a quiescent state. The galaxy exhibits a well-defined core, though the image resolution limits the identification of finer details within. Overall, the galaxy presents as a relatively massive, evolved system with moderate star formation activity, typical of galaxies at its redshift.
