The galaxy presents as a roughly elliptical, unresolved object with a smooth, featureless morphology. The color profile indicates a higher concentration of shorter wavelengths (bluer light) in the central region, fading to longer wavelengths towards the outer edges. This suggests a centrally concentrated population of younger, hotter stars within the core, and an older, redder population in the halo. There is no apparent disk structure or spiral arm morphology visible. The overall symmetrical shape and lack of visible disturbances suggests this galaxy is likely in a relatively stable state. Star formation activity, while present, appears subdued. There is no evidence of major merger events.
