The galaxy presents a generally smooth morphology with a slight elongation. Its light profile appears fairly concentrated towards the center, suggesting a dominant bulge component. The color is predominantly yellow to orange, indicating a stellar population dominated by older, redder stars. There is a potential for minor tidal disturbance on one side of the galaxy suggesting a possible interaction or past merger event. The galaxy lacks any obvious spiral arm structure or significant dust lanes. Overall, the galaxy appears consistent with an early-type galaxy, likely an elliptical or lenticular system, observed at an estimated redshift. The object may be a pair of galaxies merging but without more imaging, that is difficult to confirm.
