The galaxy appears to be a relatively smooth, elliptical type. It displays a concentrated central bulge with a noticeable decrease in light intensity towards its outer edges. There is a subtle elongation, suggesting it is not perfectly spherical, but more of a flattened spheroid shape. The color profile suggests an older stellar population; a yellow-red hue dominates the central region, indicative of evolved stars. There is minimal evidence of spiral arm structure or dust lanes. A very slight blue tint is observed at the edges which might suggest a small amount of more recent star formation. Overall, the galaxy shows a largely undisturbed morphology with no obvious signs of major mergers or tidal distortions.
