The galaxy appears to be a relatively smooth, centrally concentrated object. Its light profile suggests a spheroidal morphology, with a high degree of roundness. There is a noticeable color gradient, with the central region exhibiting a yellowish-white hue, suggesting an older stellar population. The outer regions appear dimmer and slightly redder. There is no clear evidence of spiral arm structure or significant dust lanes. The galaxy's overall appearance does not indicate a recent major merger event, although there may be some minor tidal disturbances or interactions that are difficult to discern at this resolution. The object displays a color profile suggesting a lack of significant ongoing star formation. The lack of blue light indicates that there are not many young, massive stars present. The galaxy's apparent size suggests it is a moderately sized object with a certain level of mass and luminosity.
