The galaxy appears to be a relatively compact system, likely an elliptical or lenticular galaxy based on its overall smooth appearance. It has a centrally concentrated luminosity profile, with a gradual decrease in brightness outwards. The galaxy exhibits a bluish hue, suggesting the presence of a population of young, hot stars, although the star formation rate is likely subdued. The shape of the galaxy is generally round. There is some evidence of a potential minor disturbance or interaction affecting the system, possibly related to a nearby object. There is the suggestion of a merger taking place, perhaps in its later stages. The galaxy exhibits low specific star formation rate, placing it within the population of relatively quiescent galaxies at its redshift.
