The galaxy presents an elliptical morphology, with a high degree of central concentration. The galaxy exhibits a notable bulge, which appears relatively smooth and featureless, with the light being more concentrated towards the center. The disk appears moderately inclined to the line of sight, as indicated by its oval shape. There is a color gradient apparent, with the central regions displaying a yellowish hue, suggestive of an older stellar population, while the outer regions exhibit a bluer tint. The disk does not show well-defined spiral arms. The galaxy appears to be relatively isolated, with no obvious signs of ongoing or recent major merger events. Overall, the galaxy appears to be an early-type spiral or a lenticular galaxy.