The galaxy presents a generally elliptical morphology, appearing mostly smooth and rounded. The central bulge exhibits a higher surface brightness, with colors trending toward the redder end of the spectrum, indicating a population of older stars. Emanating from the central region is a fainter disk component. There is an irregular feature protruding from the side of the galaxy, possibly indicating an ongoing or recent minor interaction or disturbance. The disk shows a degree of flattening, with the major axis extended relative to the minor axis, but the axial ratio is quite high, indicating it is more circular than elongated. Overall, the galaxy appears to be at an intermediate redshift, and its color profile suggests a moderately evolved system with ongoing or recently-terminated star formation.
