The galaxy presents an elongated, cigar-shaped morphology. The light distribution suggests a centrally concentrated spheroid, with a smooth appearance lacking distinct spiral arm features. A subtle color gradient is observed, with the core exhibiting a slightly redder hue compared to the outer regions. This could indicate an older stellar population dominating the central bulge. Given the observed redshift, the galaxy is at a significant distance. Assuming the reported redshift value, we are looking at light that has traveled a considerable distance, providing a glimpse into the galaxy's past. The absence of prominent dust lanes and well-defined spiral arms, combined with the elliptical shape, hints that this is a well evolved galaxy with relatively low current star formation. Some slight asymmetry may indicate a potential minor interaction or disturbance but there isn't any strong indication of it. The estimated mass is about 10^9.5 solar masses, which would be considered average for a galaxy with low star formation.
