The galaxy presents an elliptical morphology, with a smooth and concentrated central bulge that appears yellowish in color, suggesting an older stellar population dominating the core. Extending outwards from the central bulge, there's a fainter, more diffuse disk component. This disk exhibits a bluer hue, potentially indicative of more recent star formation activity compared to the bulge. The galaxy shows no strong signs of major disturbances or tidal features. There is a slight irregularity in the disk suggesting minor disturbances.