This galaxy presents as a relatively smooth, disk-dominated system with some disturbed features. The core region appears spheroidal and more luminous, gradually diffusing into a fainter, elongated disk. The color distribution indicates the presence of both older stellar populations in the central region and younger, bluer stars within the disk. Irregularities in the outer regions of the disk suggest minor gravitational interactions or disturbances. The overall morphology suggests a system that is likely undergoing relatively quiescent evolution with a low rate of star formation.
