The galaxy appears as a smooth, elongated structure with a high degree of central concentration. Its overall shape suggests an elliptical morphology, although there may be a faint disk component present at a slight inclination. The color profile is mostly uniform across the galaxy, with a slight reddening toward the central bulge. There is no evidence of strong spiral arms or active star formation regions. The galaxy does not appear to be undergoing any major merging events or tidal disturbances.