The galaxy presents as a moderately luminous, elliptical morphology at a redshift of approximately 0.22. Its light profile is dominated by a smooth, centrally concentrated spheroid component exhibiting a radial color gradient, with the core appearing yellow shifting toward redder hues in the outer regions, indicating the presence of an older stellar population. It does not show any evidence of spiral arms or a prominent disk structure. The general uniformity suggests a system that has largely completed the merging process. There are hints of tidal disturbances or minor interactions, but it presents predominantly as a quiescent system. The estimated size is approximately 6 kpc, suggesting a galaxy of considerable mass. Evidence of some ongoing star formation, although likely at a relatively low rate, is apparent. The galaxy can be characterized as a relatively massive, early-type system transitioning into a passive evolutionary phase.
