The galaxy presents a generally smooth appearance, with an elliptical morphology. The object has a high degree of central concentration, suggesting a prominent bulge. The light distribution reveals a color gradient, with the central region exhibiting a yellowish hue that transitions to a bluer color towards the outer edges. This color change indicates a possible difference in stellar populations, with older, redder stars dominating the core and younger, bluer stars populating the outer regions, or perhaps varying dust content across the galaxy. The galaxy appears elongated, indicating that it is either a flattened elliptical or a disk galaxy seen at an oblique angle. No obvious spiral arms or prominent dust lanes are visible, reinforcing the possibility of an elliptical nature, though a very faint disk cannot be ruled out based solely on this image. There is no obvious evidence of tidal features or recent merger activity in this image.
