The galaxy presents as a relatively bright, somewhat elongated structure. A central bulge is visible with a high degree of smoothness, suggesting a significant population of older stars. Surrounding the bulge is a disk component that appears less defined, though subtle features and disturbances are present. The overall color indices indicate a galaxy with ongoing star formation, with the disk component likely hosting younger stellar populations compared to the bulge. The galaxy shows a slight asymmetry, suggesting possible minor tidal interactions or internal dynamical processes. The general morphology indicates a galaxy that is neither perfectly elliptical nor fully spiral, occupying an intermediate position.
