The galaxy presents a smooth, elliptical morphology. It appears centrally concentrated with a noticeable decrease in luminosity moving outward from the core. The color profile suggests an older stellar population, exhibiting a yellowish-orange hue. There is no apparent spiral arm structure or dust lane obscuration. The overall form is consistently rounded, lacking any significant distortions or tidal features indicative of recent major merger activity. There are no distinct star forming regions. Light distribution implies a relatively evolved system, likely nearing the red sequence. The galaxy demonstrates a high degree of central spheroidal symmetry, with no substantial deviations from a smooth, elliptical shape.
