The observed galaxy exhibits a morphology indicative of a late-stage spiral or an elliptical galaxy with a bulge. The central region of the galaxy is characterized by a bright, concentrated spheroid component, potentially indicative of an older stellar population. A disk component is visible, with asymmetry evident. The ellipticity of the isophotes suggests a non-circular shape and a mild degree of inclination to our line of sight. The galaxy has a red color and an average size, suggesting a substantial population of evolved stars. There is an asymmetry in the disk, but no obvious signs of interaction with other galaxies.