The galaxy appears as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is a subtle gradation in brightness from the core outwards. The color profile suggests a higher concentration of older stars, with yellowish-white hues dominating the central regions. Fainter, bluer regions extend from the core, indicating ongoing star formation. The galaxy does not show any prominent spiral arms or other disk features. It shows no signs of major disturbances. The overall appearance is consistent with an evolved system with a moderate rate of star formation.