The galaxy presents an elliptical morphology. The core exhibits a concentrated, yellowish hue, suggesting an older stellar population and minimal ongoing star formation in the central region. Moving outwards from the center, a subtle shift toward greenish-blue tones is observed in the outer regions. It could be evidence of pockets of younger, hotter stars within a disk or faint spiral arms. The galaxy has a smooth appearance overall, with no visually prominent dust lanes or tidal features indicating recent major mergers or strong gravitational interactions. The galaxy appears moderately inclined relative to our line of sight, giving it a flattened, oval shape.
