This galaxy exhibits an elliptical morphology, appearing largely smooth and spheroidal in shape, with a prominent central bulge. The light distribution suggests an older stellar population, particularly within the central region, with a yellowish hue characteristic of evolved stars. Fainter, bluer regions indicate the presence of some ongoing star formation, concentrated away from the central bulge, perhaps in a faint, disturbed disk. There are signs of a possible tidal tail or disturbance in the galaxy's structure, potentially indicating an interaction with another galaxy, although no obvious companion is visible in the immediate vicinity. Overall, the galaxy appears to be a moderately massive system at intermediate redshift, likely undergoing a transition phase in its evolutionary history.
