The galaxy presents a generally smooth morphology, with a high concentration of light towards the center, suggesting a prominent bulge. Its shape is elliptical, appearing elongated rather than perfectly spherical. While there is a suggestion of a disk, it is not the dominant feature of the galaxy. No obvious spiral arm structure is discernible. There appears to be no signs of a recent or ongoing major merger event, though there is a subtle indication of minor disturbance to its structure. The galaxy exhibits a color gradient, with the central region appearing more yellowish-white compared to the outer regions, which have a slightly redder hue. This could indicate an older stellar population towards the center and younger, hotter stars in the outer regions.