The galaxy presents as an elongated, spindle-shaped object. Its central region exhibits a high concentration of light, appearing generally smooth in texture. The color profile suggests a composition of older stars, indicated by a yellowish-orange hue at the center. Fainter regions extend outward from the central bulge. These regions are more diffuse, with a hint of blue which could indicate the presence of regions with younger star formation, though the effect is not overly pronounced. There is a slight asymmetry in the distribution of the outer regions, but overall the galaxy does not show signs of major recent interaction or disturbance. Its morphology is broadly consistent with that of an elliptical galaxy or potentially an edge-on spiral galaxy, however the limited resolution prevents making a definitive classification.
