The galaxy presents a largely smooth morphology. The central region exhibits a higher luminosity and a yellow-white hue, which is indicative of an older stellar population. A faint, diffuse blue halo surrounds the central bulge, suggesting the presence of some younger, hotter stars, though these are not prominent. The overall shape is nearly circular. No distinct spiral arms or bar structures are apparent. There is no evidence of significant tidal disturbances or ongoing merger activity. The galaxy displays a relatively uniform light distribution, with a gradual decrease in brightness from the core outwards.
