The galaxy appears as a relatively smooth, elliptical-shaped structure, with a concentrated central bulge. The light distribution suggests a dominance of older stellar populations, exhibiting a yellowish hue in the core region. A subtle gradient in color is observable, transitioning to slightly bluer tones in the outer regions, potentially indicating the presence of some younger stars, or a shell structure resulting from a past merger. However, there is no clear evidence of ongoing, high star formation activity, and the morphology is generally undisturbed. The overall shape is close to circular but not perfectly so, with a subtle elongation suggesting a deviation from a perfect spherical form. The galaxy does not appear to be undergoing any major mergers or interactions.
