This galaxy presents a relatively smooth, elliptical morphology. The central region exhibits a high degree of luminosity, appearing bright yellow-white in color, suggesting an older stellar population. Moving outward from the core, the luminosity gradually decreases. A faint, bluish halo surrounds the core, possibly indicating the presence of some younger, hotter stars, or low level ongoing star formation within the disk. There is no distinct spiral arm structure visible; the overall form appears largely featureless, consistent with an elliptical galaxy classification. No obvious signs of major merging events or significant tidal disturbances are readily apparent in the image. The axial ratio suggests the galaxy is nearly circular but slightly elongated.
