The galaxy presents as a generally smooth, elliptical morphology. There is a notable concentration of light towards the galactic center, exhibiting a yellowish-orange hue indicative of an older stellar population. The light becomes more diffuse towards the outer regions of the galaxy. A subtle blue tinge is visible in these outer regions suggesting the presence of some younger, hotter stars, possibly in regions of recent or ongoing star formation. Overall the shape is generally round, though not perfectly so. There appears to be some minor irregularity in the structure, though no major distortions or signs of recent mergers are immediately apparent.
