The observed galaxy appears to be a relatively smooth, elliptical galaxy, with no prominent spiral arms or bar structure visible in this image. The light distribution suggests a centrally concentrated luminosity profile. There's a significant color gradient, appearing yellower toward the center, indicating an older stellar population and likely a higher concentration of metals in the core region. The outer regions of the galaxy exhibit a bluer hue, potentially indicative of a sparse population of younger, hotter stars, but more likely is due to noise. The galaxy is mostly symmetrical, exhibiting a round morphology. No apparent signs of tidal disturbances or ongoing major merger events are detected. Based on the data, this galaxy has a redshift of approximately 0.15, placing it at a considerable distance. Estimated size is roughly 4 kpc. This galaxy has an estimated mass of 10^10 solar masses. The low estimated star formation rate suggests it may be undergoing quenching, or that it could have a low rate of star formation.
