The galaxy appears as a relatively smooth, elliptical structure, exhibiting a high degree of central concentration. Its overall shape is generally round, with no discernible spiral arms or a distinct disk component visible at this resolution. The color profile is dominated by a yellow-orange hue, suggesting a population of older stars, although the presence of some blue light hints at a lower level of ongoing star formation. There is no obvious evidence of significant tidal disturbances or ongoing mergers; the galaxy appears relatively undisturbed. The galaxy is rather compact, with light concentrated toward the center.
