The galaxy presents as a centrally concentrated, smooth object with a generally elliptical morphology. There is no obvious spiral structure or distinct features such as bars or rings. The light distribution appears largely uniform, exhibiting a radial gradient with the brightest region concentrated towards the galactic center, which fades smoothly into the surrounding background. The color profile is dominated by a yellowish-orange hue, suggesting a population of older stars and a relatively low rate of ongoing star formation. There may be some minor irregularities or a slight asymmetry in the outer regions, but these are not pronounced. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
