This galaxy presents a relatively smooth, elliptical morphology. The light is concentrated towards the center, indicating a prominent bulge. There is a faint bluish hue to the extended halo of the galaxy, suggesting the presence of some young stars or ongoing star formation, although the overall rate appears to be relatively low. The galaxy appears to be fairly isolated, with no obvious signs of major mergers or tidal disturbances. The overall shape is rounded with no prominent features, such as spiral arms, visible in this image. There might be some very minor irregularities in the outer regions, perhaps hinting at past interactions or subtle internal structure.
