The galaxy appears to be an elliptical galaxy at a redshift of approximately 0.12, suggesting significant distance. It exhibits a largely smooth morphology with a near-spherical shape, showing no clear evidence of spiral arms or a defined disk structure. The central region is characterized by high luminosity, with a concentrated stellar population. The color profile indicates a redder hue, likely indicative of an older stellar population and/or significant dust obscuration. There is no apparent indication of on-going major merging events or tidal disturbances. The galaxy appears relatively isolated, without nearby companions that would suggest significant gravitational interaction. Its estimated effective radius is approximately 2.5 kpc.
