The galaxy presents as a centrally concentrated, luminous object, exhibiting a relatively smooth, elliptical morphology. Its overall shape is more rounded than elongated, with a slight deviation from perfect circularity. There is no visible spiral structure or evidence of a prominent disk component. The color profile indicates a generally bluer central region, gradually transitioning towards a redder hue in the outer regions, which may be due to varying stellar populations. No major disturbances or merger events are apparent, although subtle irregularities in the outer halo may suggest minor interactions in the past. The galaxy exhibits an estimated size of approximately 5 kpc across and a likely mass of approximately 10^10 solar masses, with relatively modest rates of ongoing star formation.
