This galaxy appears to be a relatively smooth, elliptical-like system. It exhibits a bright, concentrated central bulge region displaying a yellowish hue, likely indicating an older stellar population. The galaxy's outer regions show a more diffuse, bluish color, potentially suggesting the presence of younger stars or ongoing star formation, although the overall star formation rate appears low. There is some evidence of minor disturbances within the galaxy, hinting at the possibility of past or ongoing interactions or mergers. The overall shape is roughly rounded but slightly elongated and somewhat irregular, possibly influenced by internal dynamics or external interactions. There is a hint of a disk-like feature.
