The galaxy exhibits a generally elliptical morphology, appearing moderately smooth with a dominant central bulge. There are hints of a disk component. Evidence suggests the galaxy is undergoing a merging event or has experienced a recent interaction, as indicated by the asymmetrical distribution of light and subtle distortions in its overall shape. The galaxy’s color profile is predominantly yellow, suggesting an older stellar population. However, bluer regions indicate ongoing star formation, albeit at a moderate rate. The galaxy exhibits an estimated effective radius of approximately 6 kpc. The galaxy demonstrates a substantial stellar mass, likely within the range of 10^10 to 10^11 solar masses. The specific star formation rate is relatively low suggesting it may be in a transition phase.
