The galaxy appears as a moderately bright, flattened spheroid. The core exhibits a concentrated yellowish-orange hue, suggesting a significant population of older stars. Extending outward from the core is a less defined region of diffuse light, appearing slightly greener in tone. This suggests the presence of a more distributed population of younger stars or regions of ongoing star formation, although this activity is not pronounced. There are no immediately obvious spiral arm structures. The overall morphology leans toward a smooth, elliptical galaxy, with a subtle hint of a disk-like component or perhaps a mild disturbance event influencing its structure. The galaxy's shape is neither perfectly round nor highly elongated, placing it somewhere between a spherical and cigar-shaped form. There is no strong evidence of a major ongoing merger, although minor disturbances or interactions cannot be ruled out based on visual inspection.