The galaxy presents as a smooth, elliptical morphology, with no apparent spiral arm structure or prominent dust lanes. The light distribution suggests a centrally concentrated spheroid, gradually fading toward the edges. It is elongated in shape, appearing cigar-shaped with axial symmetry. There is minimal evidence of tidal disturbances or ongoing major mergers with other galaxies. The color profile appears relatively uniform across the galaxy, suggesting a lack of significant recent star formation activity. The overall appearance is consistent with that of an evolved galaxy with an older stellar population. The light emitted is primarily concentrated in the green, red and z-band.
