The galaxy presents a generally smooth and elliptical morphology. Its light profile appears concentrated towards the center, indicating a significant bulge component. Some subtle disk features are present, but they are not prominent. The color gradient transitions from a somewhat bluer hue in the outer regions to a redder hue in the core. There is no obvious evidence of tidal disturbances or ongoing major mergers. The galaxy has a mostly rounded shape, and a minor amount of disturbance to the structure. Based on its redshift, this galaxy is at an intermediate distance. The color suggests a mix of stellar populations, with older, redder stars dominating the bulge and potentially younger, bluer stars in the outer regions, suggesting a low level of ongoing star formation.
