The galaxy presents an overall elliptical morphology, elongated along a major axis. Its structure appears predominantly smooth, with a high concentration of light towards the galactic center, indicating a prominent bulge. The luminosity profile transitions smoothly from the core outward. Color gradients are observed; the central bulge exhibits a yellowish-orange hue, suggesting an older stellar population, while the outer regions display a bluer tint, which may indicate the presence of younger, hotter stars or ongoing star formation. There is subtle suggestion of a disk structure with some faint features. There is no strong evidence of any major mergers or significant tidal disturbances in its vicinity.
