The galaxy presents as a luminous, centrally concentrated system. Its overall morphology appears relatively smooth, with a high degree of central brightness. There is some evidence of a slight ellipticity, neither perfectly round nor highly elongated. No prominent spiral arm structures or dust lanes are immediately visible. There may be some minor disturbances in the disk, though nothing indicative of a major interaction. The color profile shifts from yellow-white at the central bulge to slightly redder hues in the outer regions. This color gradient suggests a possible radial variation in stellar populations or dust content.
