This galaxy appears to be a relatively smooth, disk-like structure, with a possible spheroidal component. It presents a somewhat elongated shape. The galaxy's color is predominantly a slightly bluer hue, with a fainter redder core which could suggest an older stellar population. This galaxy may be undergoing some low levels of star formation within the disk. There may be minor disturbances, but no large-scale disruptions from merging activity is evident. The galaxy's redshift indicates a distance where the galaxy's size is approximately 4.5 kpc. The estimated stellar mass is around 10^10 solar masses, with a specific star formation rate of ~10^-10 per year, which suggests a relatively quiescent star formation activity. The morphology suggests this galaxy is undergoing a transition phase between spiral and elliptical morphology.
