The galaxy presents as a system with an estimated redshift of approximately 0.24. Morphologically, it appears somewhat smooth in the central regions, with a possible faint disk-like structure or other feature extending outward. The overall shape exhibits a degree of roundness, though it deviates from being perfectly circular. Indications suggest that there may be some form of interaction, possibly a minor disturbance or ongoing merger event. The color profile indicates a relatively strong presence of red light, suggesting a population dominated by older stars. The galaxy exhibits a relatively high star formation rate, suggesting it could be a moderately active galaxy at its redshift.
