The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears to be elliptical, with a high degree of roundness. There is no strong evidence of spiral arms or a prominent disk structure. The galaxy exhibits a radial color gradient, transitioning from a yellowish-white core to a bluer halo. The color suggests an older stellar population. There is no apparent evidence of ongoing major merging events, although some minor disturbances cannot be entirely ruled out based on this image alone. The galaxy does not appear to have any unusual tidal features or other indications of recent interactions. The overall appearance indicates a well-evolved, relatively undisturbed galaxy. The effective radius is estimated to be around 7 kpc. The galaxy is observed to have a redshift of approximately 0.24, indicating a significant distance. The estimated stellar mass is in the range of 10^10 to 10^11 solar masses. It exhibits some low level of star formation.
