This galaxy appears to be an intermediate-type system, exhibiting characteristics of both elliptical and spiral morphologies. It is largely smooth in appearance, with approximately 70% of classifications identifying it as such. The system is somewhat round.

There is evidence of potential interactions or disturbances. Approximately 19% of classifications suggest minor disturbances and 20% for major disturbances in the morphology of the system. A significant amount of the classification suggests that it is undergoing a merger.

The galaxy exhibits a color gradient, appearing bluer in the outer regions. The center of the galaxy appears more redshifted, suggesting an older stellar population in the bulge. The bluer color in the outer regions may indicate regions of active star formation.
