The galaxy appears to be at an intermediate redshift. It exhibits a generally smooth morphology with a moderate central concentration. There is some indication of a disk-like structure, or potentially some irregularity indicating possible tidal disturbance or ongoing interaction. The galaxy displays a color gradient, appearing bluer towards the center and transitioning to redder hues in the outer regions. The bluer color suggests the presence of younger stellar populations and ongoing star formation activity, particularly in the central region, while the redder colors indicate older stellar populations in the galaxy's outskirts. There is a possibility of a minor merging event, with some observed disturbances in its shape. It is difficult to assess the presence of spiral arms due to the galaxy's inclination and resolution of the image. The galaxy is of moderate size and luminosity.
