The galaxy presents an overall elliptical morphology, displaying a smooth, diffuse appearance with a high degree of central concentration. The light distribution suggests an oblate spheroid shape, observed nearly edge-on. A prominent bulge dominates the central region, exhibiting a bright, concentrated core. The surrounding halo appears significantly fainter and more extended. Subtle color gradients are observed; the central bulge exhibits a slightly redder hue, while the outer regions show a subtle shift towards bluer tones. No distinct spiral arms or prominent dust lanes are discernible, although there are some vague features to be seen. Based on the color distribution, the central bulge likely consists of an older stellar population compared to the outer regions, indicating a possible age gradient within the galaxy. Minor disturbances can be seen, but no evidence of a major merger.
